邻近恒星列表

这份清单包含距离太阳系6.13秒差距（20光年）内所有已知的恒星和棕矮星。除了太阳系之外，目前已知在这个距离内还有94个恒星系统。这些系统共包含103颗进行氢融合的恒星（其中80颗是红矮星）、21颗棕矮星和6颗白矮星。尽管这些天体相对而言都很接近地球，但是只有22颗的视星等小于6.5等，这意味着这些天体只有大约21%是可以用裸眼看见^[1]。除了太阳之外，只有三颗是明亮的1等星：南门二（半人马座α星）、天狼星（大犬座α星）、和南河三（小犬座α星）。这些天体全部都位于银河系猎户臂的本地泡。

此短片显示邻近太阳周围的恒星。

恒星距离表

备注
$	亮星 (绝对星等为+8.5或更低)
‡	白矮星
§	棕矮星
&	次棕矮星或流浪行星
#	肉眼可见 (视星等为+6.5或更低)

#	名称		恒星类型	视星等	绝对星等	有效温度（±）（K）	历元 J2000.0		视差^[2]^[3]（±）（角秒）	距离^[4]（±）（光年）	附加参考资料及备注
#	系统	恒星	恒星类型	视星等	绝对星等	有效温度（±）（K）	赤经^[2]	赤纬^[2]	视差^[2]^[3]（±）（角秒）	距离^[4]（±）（光年）	附加参考资料及备注
	太阳系	太阳	G2V^[2]	−26.72^[2]#	4.85^[2]	5,778^[5]	—	—	180°	0.0000158（3）（大约8光分）
1	南门二（Rigil Kentaurus; Toliman）	半人马座比邻星（V645 Centauri）	M5.5Ve	11.09^[2]	15.53^[2]	3,040^[6]	14^h 29^m 43.0^s	−62° 40′ 46″	0.768 87（0 29）″^[7]^[8]	4.2421（16）	^[9]拥有3个行星﹙b，c，d﹚
		半人马座αA（HD 128620）	G2V^[2]	0.01^[2]#	4.38^[2]	5,790^[6]	14^h 39^m 36.5^s	−60° 50′ 02″	0.747 23（1 17）″^[7]^[10]	4.3650（68）
		半人马座αB（HD 128621）	K0V^[2]	1.34^[2]#	5.71^[2]	5,260^[6]	14^h 39^m 35.1^s	−60° 50′ 14″	0.747 23（1 17）″^[7]^[10]	4.3650（68）
2	巴纳德星（BD+04°3561a）		M4.0Ve	9.53^[2]	13.22^[2]	3,134(102)^[11]	17^h 57^m 48.5^s	+04° 41′ 36″	0.546 98（1 00）″^[7]^[8]	5.9630（109）
3	Luhman 16	WISE 1049-5319A	L8	10.73 ± 0.03			10^h 49^m 15.57^s	−53° 19′ 06″	0.496 (37)^[12]	6.52（49）
3	Luhman 16	WISE 1049-5319B	L9/T0？				10^h 49^m 15.57^s	−53° 19′ 06″	0.496 (37)^[12]	6.52（49）
3	WISE_0855–0714		Y4	25		240	08^h 55^m 10.83^s	-07° 14′ 42.5″	0.439 ″^[13]	7.43
3	沃夫359（CN Leonis）		M6.0V^[2]	13.44^[2]	16.55^[2]	2,800(100)^[14]	10^h 56^m 29.2^s	+07° 00′ 53″	0.419 10（2 10）″^[7]	7.7825（390）
4	拉兰德21185（BD+36°2147）		M2.0V^[2]	7.47^[2]	10.44^[2]	3,400^[15]	11^h 03^m 20.2^s	+35° 58′ 12″	0.393 42（0 70）″^[7]^[8]	8.2905（148）	拥有2个行星
5	天狼星（大犬座α）	天狼星A	A1V^[2]	−1.43^[2]#	1.47^[2]	9,940(210)^[16]	06^h 45^m 08.9^s	−16° 42′ 58″	0.380 02（1 28）″^[7]^[8]	8.5828（289）
5	天狼星（大犬座α）	天狼星B‡	DA2^[2]	8.44^[2]	11.34^[2]	25,000(200)^[17]	06^h 45^m 08.9^s	−16° 42′ 58″	0.380 02（1 28）″^[7]^[8]	8.5828（289）
6	鲁坦726-8	鲁坦 726-8 A（鲸鱼座BL）	M5.5Ve	12.54^[2]	15.40^[2]	2,670	01^h 39^m 01.3^s	−17° 57′ 01″	0.373 70（2 70）″^[7]	8.7280（631）
6	鲁坦726-8	鲁坦 726-8 B（鲸鱼座UV）	M6.0Ve	12.99^[2]	15.85^[2]	~2,600	01^h 39^m 01.3^s	−17° 57′ 01″	0.373 70（2 70）″^[7]	8.7280（631）
6.5	WISE 1541-2250		Y0	21.16±0.36	20.99±0.52		15^h 41^m 51.57^s	−22° 50′ 25.03″	0.351″ ± 0.108″^[18]	9.3 +4.1/–2.2^[18]
7	罗斯154（V1216 Sagittarii）		M3.5Ve	10.43^[2]	13.07^[2]	2,700	18^h 49^m 49.4^s	−23° 50′ 10″	0.336 90（1 78）″^[7]^[8]	9.6813（512）
8	罗斯248（HH Andromedae）		M5.5Ve	12.29^[2]	14.79^[2]	?	23^h 41^m 54.7^s	+44° 10′ 30″	0.316 00（1 10）″^[7]	10.322（36）
9	天苑四（BD−09°697）		K2V^[2]	3.73^[2]#	6.19^[2]	5,100	03^h 32^m 55.8^s	−09° 27′ 30″	0.309 99（0 79）″^[7]^[8]	10.522（27）	拥有1个行星﹙b﹚
10	拉卡伊9352（CD−36°15693）		M1.5Ve	7.34^[2]	9.75^[2]	3,340	23^h 05^m 52.0^s	−35° 51′ 11″	0.303 64（0 87）″^[7]^[8]	10.742（31）	拥有2个行星
11	罗斯128（FI Virginis）		M4.0Vn	11.13^[2]	13.51^[2]	2,800	11^h 47^m 44.4^s	+00° 48′ 16″	0.298 72（1 35）″^[7]^[8]	10.919（49）	拥有1个行星﹙b﹚
12	宝瓶座EZ （GJ 866,鲁坦 789-6）	EZ Aquarii A	M5.0Ve	13.33^[2]	15.64^[2]	?	22^h 38^m 33.4^s	−15° 18′ 07″	0.289 50（4 40）″^[7]	11.266（171）
		EZ Aquarii B	M?	13.27^[2]	15.58^[2]	?
		EZ Aquarii C	M?	14.03^[2]	16.34^[2]	?
13	南河三（小犬座α）	南河三 A	F5V-IV^[2]	0.38^[2]#	2.66^[2]	6,650	07^h 39^m 18.1^s	+05° 13′ 30″	0.286 05（0 81）″^[7]^[8]	11.402（32）
13	南河三（小犬座α）	南河三 B	DA^[2]	10.70^[2]	12.98^[2]	9,700	07^h 39^m 18.1^s	+05° 13′ 30″	0.286 05（0 81）″^[7]^[8]	11.402（32）
14	天津增二十九	61 Cygni A（BD+38°4343）	K5.0V^[2]	5.21^[2]#	7.49^[2]	4,640	21^h 06^m 53.9^s	+38° 44′ 58″	0.286 04（0 56）″^[7]^[8]	11.403（22）
14	天津增二十九	61 Cygni B（BD+38°4344）	K7.0V^[2]	6.03^[2]#	8.31^[2]	4,440	21^h 06^m 55.3^s	+38° 44′ 31″	0.286 04（0 56）″^[7]^[8]	11.403（22）
15	Struve 2398 (GJ 725, BD+59°1915)	Struve 2398 A（HD 173739）	M3.0V^[2]	8.90^[2]	11.16^[2]	?	18^h 42^m 46.7^s	+59° 37′ 49″	0.283 00（1 69）″^[7]^[8]	11.525（69）
15	Struve 2398 (GJ 725, BD+59°1915)	Struve 2398 B（HD 173740）	M3.5V^[2]	9.69^[2]	11.95^[2]	?	18^h 42^m 46.9^s	+59° 37′ 37″	0.283 00（1 69）″^[7]^[8]	11.525（69）
16	Groombridge 34 (GJ 15)	Groombridge 34 A（GX Andromedae）	M1.5V^[2]	8.08^[2]	10.32^[2]	?	0^h 18^m 22.9^s	+44° 01′ 23″	0.280 59（0 95）″^[7]^[8]	11.624（39）	拥有2个行星
16	Groombridge 34 (GJ 15)	Groombridge 34 B（GQ Andromedae）	M3.5V^[2]	11.06^[2]	13.30^[2]	?	0^h 18^m 22.9^s	+44° 01′ 23″	0.280 59（0 95）″^[7]^[8]	11.624（39）
17	波斯七（CPD−57°10015）	Epsilon Indi A	K5Ve^[2]	4.69^[2]#	6.89^[2]	4,280	22^h 03^m 21.7^s	−56° 47′ 10″	0.275 84（0 69）″^[7]^[8]	11.824（30）	拥有1个行星
		Epsilon Indi Ba	T1.0V	>23	>25	1,280	22^h 04^m 10.5^s	−56° 46′ 58″
		Epsilon Indi Bb	T6.0V	>23	>25	850	22^h 04^m 10.5^s	−56° 46′ 58″
18	巨蟹座DX（G 51-15）		M6.5Ve	14.78^[2]	16.98^[2]	?	08^h 29^m 49.5^s	+26° 46′ 37″	0.275 80（3 00）″^[7]	11.826（129）
19	天仓五（BD−16°295）		G8Vp^[2]	3.49^[2]#	5.68^[2]	5,344	01^h 44^m 04.1^s	−15° 56′ 15″	0.274 39（0 76）″^[7]^[8]	11.887（33）	拥有7个行星
20	GJ 1061（LHS 1565）		M5.5V^[2]	13.09^[2]	15.26^[2]	?	03^h 35^m 59.7^s	−44° 30′ 45″	0.272 01（1 30）″^[19]	11.991（57）	^[20]^[21]拥有3个行星
21	鲸鱼座YZ星（LHS 138）		M4.5V^[2]	12.02^[2]	14.17^[2]	?	01^h 12^m 30.6^s	−16° 59′ 56″	0.268 84（2 95）″^[7]^[8]	12.132（133）
22	鲁坦星（BD+05°1668）		M3.5Vn	9.86^[2]	11.97^[2]	?	07^h 27^m 24.5^s	+05° 13′ 33″	0.263 76（1 25）″^[7]^[8]	12.366（59）	拥有2个行星
23	蒂加登星（SO025300.5+165258）		M6.5V	15.14^[2]	17.22^[2]	?	02^h 53^m 00.9^s	+16° 52′ 53″	0.260 63（2 69）″^[19]	12.514（129）	^[21]拥有2个行星
24	SCR 1845-6357	SCR 1845-6357 A	M8.5V^[2]	17.39	19.41	?	18^h 45^m 05.3^s	−63° 57′ 48″	0.259 45（1 11）″^[19]	12.571（54）	^[21]
24	SCR 1845-6357	SCR 1845-6357 B	T6^[22]	?	?	950^[22]	18^h 45^m 02.6^s	−63° 57′ 52″	0.259 45（1 11）″^[19]	12.571（54）	^[21]
25	卡普坦星（CD−45°1841）		M1.5V^[2]	8.84^[2]	10.87^[2]	3,800	05^h 11^m 40.6^s	−45° 01′ 06″	0.255 27（0 86）″^[7]^[8]	12.777（43）	拥有2个行星
26	Lacaille 8760（AX Microscopii）		M0.0V^[2]	6.67^[2]	8.69^[2]	3,340	21^h 17^m 15.3^s	−38° 52′ 03″	0.253 43（1 12）″^[7]^[8]	12.870（57）
27	Kruger 60 （BD+56°2783）	Kruger 60 A	M3.0V^[2]	9.79^[2]	11.76^[2]	3,180	22^h 27^m 59.5^s	+57° 41′ 45″	0.248 06（1 39）″^[7]^[10]	13.149（74）
27	Kruger 60 （BD+56°2783）	Kruger 60 B（DO Cephei）	M4.0V^[2]	11.41^[2]	13.38^[2]	2,890	22^h 27^m 59.5^s	+57° 41′ 45″	0.248 06（1 39）″^[7]^[10]	13.149（74）
28	DEN 1048-3956		M8.5V^[2]	17.39^[2]	19.37^[2]	?	10^h 48^m 14.7^s	−39° 56′ 06″	0.247 71（1 55）″^[19]	13.167（82）	^[23]^[24]
29	罗斯614 （V577 Monocerotis, GJ 234）	Ross 614A（LHS 1849）	M4.5V^[2]	11.15^[2]	13.09^[2]	?	06^h 29^m 23.4^s	−02° 48′ 50″	0.244 34（2 01）″^[7]^[10]	13.349（110）
29	罗斯614 （V577 Monocerotis, GJ 234）	Ross 614B（LHS 1850）	M5.5V	14.23^[2]	16.17^[2]	?	06^h 29^m 23.4^s	−02° 48′ 50″	0.244 34（2 01）″^[7]^[10]	13.349（110）
30	Gl 628（Wolf 1061, BD−12°4523）		M3.0V^[2]	10.07^[2]	11.93^[2]	?	16^h 30^m 18.1^s	−12° 39′ 45″	0.236 01（1 67）″^[7]^[8]	13.820（98）	拥有3个行星﹙b，c，d﹚
31	范马南星（Gl 35, LHS 7）		DZ7^[2]	12.38^[2]	14.21^[2]	?	00^h 49^m 09.9^s	+05° 23′ 19″	0.231 88（1 79）″^[7]^[8]	14.066（109）
32	格利泽1（CD−37°15492）		M3.0V^[2]	8.55^[2]	10.35^[2]	?	00^h 05^m 24.4^s	−37° 21′ 27″	0.229 20（1 07）″^[7]^[8]	14.231（66）
33	沃夫424 （室女座FL，LHS 333, GJ 473）	Wolf 424 A	M5.5Ve	13.18^[2]	14.97^[2]	?	12^h 33^m 17.2^s	+09° 01′ 15″	0.227 90（4 60）″^[7]	14.312（289）
33	沃夫424 （室女座FL，LHS 333, GJ 473）	Wolf 424 B	M7Ve	13.17^[2]	14.96^[2]	?	12^h 33^m 17.2^s	+09° 01′ 15″	0.227 90（4 60）″^[7]	14.312（289）
34	白羊座TZ（GJ 83.1, Luyten 1159-16）		M4.5V^[2]	12.27^[2]	14.03^[2]	?	02^h 00^m 13.2^s	+13° 03′ 08″	0.224 80（2 90）″^[7]	14.509（187）	拥有1个行星
35	Gl 687（LHS 450, BD+68°946）		M3.0V^[2]	9.17^[2]	10.89^[2]	?	17^h 36^m 25.9^s	+68° 20′ 21″	0.220 49（0 82）″^[7]^[8]	14.793（55）	拥有2个行星
36	LHS 292（LP 731-58）		M6.5V^[2]	15.60^[2]	17.32^[2]	?	10^h 48^m 12.6^s	−11° 20′ 14″	0.220 30（3 60）″^[7]	14.805（242）
37	Gl 674（LHS 449）		M3.0V^[2]	9.38^[2]	11.09^[2]	?	17^h 28^m 39.9^s	−46° 53′ 43″	0.220 25（1 59）″^[7]^[8]	14.809（107）	拥有1个行星
38	GJ 1245	GJ 1245 A	M5.5V^[2]	13.46^[2]	15.17^[2]	?	19^h 53^m 54.2^s	+44° 24′ 55″	0.220 20（1 00）″^[7]	14.812（67）
		GJ 1245 B	M6.0V^[2]	14.01^[2]	15.72^[2]	?	19^h 53^m 55.2^s	+44° 24′ 56″
		GJ 1245 C	M?	16.75^[2]	18.46^[2]	?	19^h 53^m 54.2^s	+44° 24′ 55″
39	GJ 440（WD 1142-645）		DQ6^[2]	11.50^[2]	13.18^[2]	7,500	11^h 45^m 42.9^s	−64° 50′ 29″	0.216 57（2 01）″^[7]^[8]	15.060（140）
40	GJ 1002		M5.5V^[2]	13.76^[2]	15.40^[2]	?	00^h 06^m 43.8^s	−07° 32′ 22″	0.213 00（3 60）″^[7]	15.313（259）	拥有2个行星
41	罗斯780（GJ 876）		M3.5V^[2]	10.17^[2]	11.81^[2]	3,480	22^h 53^m 16.7^s	−14° 15′ 49″	0.212 59（1 96）″^[7]^[8]	15.342（141）	拥有4个行星﹙b，c，d，e﹚
42	LHS 288（Luyten 143-23）		M5.5V^[2]	13.90^[2]	15.51^[2]	?	10^h 44^m 21.2^s	−61° 12′ 36″	0.208 95（2 73）″^[19]	15.610（204）	^[21]
43	GJ 412	GJ 412 A	M1.0V^[2]	8.77^[2]	10.34^[2]	?	11^h 05^m 28.6^s	+43° 31′ 36″	0.206 02（1 08）″^[7]^[8]	15.832（83）
43	GJ 412	GJ 412 B（WX Ursae Majoris）	M5.5V^[2]	14.48^[2]	16.05^[2]	?	11^h 05^m 30.4^s	+43° 31′ 18″	0.206 02（1 08）″^[7]^[8]	15.832（83）
44	Groombridge 1618（GJ 380）		K7.0V^[2]	6.59^[2]	8.16^[2]	4,000	10^h 11^m 22.1^s	+49° 27′ 15″	0.205 81（0 67）″^[7]^[8]	15.848（52）
45	GJ 388		M3.0V^[2]	9.32^[2]	10.87^[2]	?	10^h 19^m 36.4^s	+19° 52′ 10″	0.204 60（2 80）″^[7]	15.942（218）
46	GJ 832		M3.0V^[2]	8.66^[2]	10.20^[2]	?	21^h 33^m 34.0^s	−49° 00′ 32″	0.202 78（1 32）″^[7]^[8]	16.085（105）	拥有1个行星﹙b﹚
47	DEN 0255-4700		L7.5V^[2]	22.92^[2]	24.44^[2]	?	02^h 55^m 03.7^s	−47° 00′ 52″	0.201 37（3 89）″^[19]	16.197（313）	^[24]
48	GJ 682		M4.5V^[2]	10.95^[2]	12.45^[2]	?	17^h 37^m 03.7^s	−44° 19′ 09″	0.199 65（2 30）″^[7]^[8]	16.337（188）
49	波江座40 (40 Eridani, Gliese 166)	Keid (A)$	K0.5V	4.43#	5.93	5,202	04^h 15^m 16.3^s	-07° 39′ 10″	0.199 69	16.34
		B‡	DA4	9.52	11.02	?	04^h 15^m 21.8^s	−07° 39′ 29″
		C	M4V	11.24	12.74	3,167	04^h 15^m 21.5^s	−07° 39′ 22″
50	蝎虎座EV		M3.5 V	10.22	11.70	3,291	22^h 46^m 49.7^s	+44° 20′ 02″	0.197 957	16.4761	恒星上所见到最明亮的闪焰事件
51	宗人四 (Gliese 702)	A$	K0V	4.21#	5.66	5,419	18^h 05^m 27.4^s	+02° 29′ 59″	0.195 2166^[25]	16.7074
51	宗人四 (Gliese 702)	B$	K5V	6.01#	7.46	4,393	18^h 05^m 27.5^s	+02° 29′ 56″	0.195 2166^[25]	16.7074
52	牛郎星 (Alpha Aquilae)$		A7 IV-Vn	0.77#	2.22	7,377	19^h 50^m 47.0^s	+08° 52′ 06″	0.194 95^[26]	16.730
53	巨蟹座EI (GJ 1116, G 9-38)	A	M5.5V	14.06	15.50	?	08^h 58^m 15.2^s	+19° 45′ 47″	0.194 1443	16.800
53	巨蟹座EI (GJ 1116, G 9-38)	B	M V	14.92	16.36	?	08^h 58^m 15.2^s	+19° 45′ 47″	0.194 1443	16.800
54	WISE J150649.97+702736.1§		T6	13.74 J	15.17 J	?	15^h 06^m 52.4^s	+70° 27′ 25″	0.193 5	16.856
55	GJ 3379 (G 99-49)		M3.5V	11.31	12.73	3,284	06^h 00^m 03.5^s	+02° 42′ 24″	0.192 0135	16.9861
56	DENIS J081730.0-615520§		T6	13.61 J	15.03 J	950	08^h 17^m 30.1^s	−61° 55′ 16″	0.191 8362	17.002
57	格利泽445 (LHS 2459, G 254-29)		M3.5V	10.79	12.19	3,369	11^h 47^m 41.4^s	+78° 41′ 28″	0.190 3251	17.1368
58	2MASS J15404342−5101357		M7V	15.26	16.63	?	15^h 40^m 43.5^s	-51° 01′ 36″	0.187 7290	17.3738
59	2MASS 0939−2448	A§	T8V	15.61 J	16.97 J	500	09^h 39^m 35.5^s	−24° 48′ 28″	0.187 3^[27]	17.41	棕矮星联星系统
59	2MASS 0939−2448	B§	T8V			?	09^h 39^m 35.5^s	−24° 48′ 28″	0.187 3^[27]	17.41	棕矮星联星系统
60	格利泽3323 (LHS 1723, LP 656-38)		M4V	12.22	13.57	3,288	05^h 01^m 57.4^s	−06° 56′ 46″	0.186 0466	17.5309	拥有2个行星
61	格利泽526 (Wolf 498, HD 119850)		M1V	8.46	9.78	3,521	13^h 45^m 43.8^s	+14° 53′ 29″	0.183 9962	17.7263
62	施泰因2051 (Gliese 169.1, G 175-34)	A	M4V	11.04	12.33	3,277	04^h 31^m 11.5^s	+58° 58′ 37″	0.181 2730	17.9925
62	施泰因2051 (Gliese 169.1, G 175-34)	B‡	DC5	12.43	13.72	7,130	04^h 31^m 12.6^s	+58° 58′ 41″	0.181 2730	17.9925
63	WISEP J111448.80-261828.2§		T7.5	15.86 J	17.12 J	750	11^h 14^m 51.3^s	−26° 18′ 24″	0.179 2^[28]	18.20
64	格利泽251 (Wolf 294, HD 265866)		M3V	10.02	11.29	3,451	06^h 54^m 49.0^s	+33° 16′ 05″	0.179 0629	18.2146	拥有1个行星
65	LP 816-60		M3.5V	11.50	12.75	3,239	20^h 52^m 33.0^s	-16° 58′ 29″	0.177 9312	18.3305
66	WISEA J183537.82+325945.4		M8.5V	18.27	19.50	2,400	18^h 35^m 37.9^s	+32° 59′ 55″	0.175 7930	18.5534
67	格利泽205 (Wolf 1453, HD 36395)		M1V	7.95	9.17	3,891	05^h 31^m 27.4^s	−03° 40′ 38″	0.175 3131	18.6042
68	WISE J041521.21-093500.6§		T8	15.34 J	16.56 J	?	04^h 15^m 19.5^s	−09° 35′ 07″	0.175 2^[28]	18.708
69	格利泽229 (HD 42581)	A	M1.5V	8.14	9.34	3,837	06^h 10^m 34.6^s	−21° 51′ 53″	0.173 5740	18.7906	拥有2个行星
69	格利泽229 (HD 42581)	B§	T6V	14.01 J	15.21 J	?	06^h 10^m 34.6^s	−21° 51′ 53″	0.173 5740	18.7906
70	天厨二 (Sigma Draconis)$		G9V	4.67#	5.87	5,338	19^h 32^m 21.6^s	+69° 39′ 40″	0.173 4939	18.7993
71	罗斯47 (Gliese 213)		M4V	11.57	12.76	3,311	05^h 42^m 09.3^s	+12° 29′ 21″	172.6762	18.8883
72	格利泽570 (Lalande 27173, 33 G. Librae)	A$	K4V	5.64#	6.79	4,625	14^h 57^m 28.0^s	-21° 24′ 56″	0.169 8843	19.1987
		B	M1.5V	8.30	9.45	4.077
		C	M	9.96	11.11	?
		D§	T7.5	15.32 J	16.47 J	500
73	格利泽693 (Luyten 205-128)		M3V	10.76	11.91	3,386	17^h 46^m 32.4^s	-57° 19′ 09″	0.169 8042	19.2078
74	葛利斯754 (Luyten 347-14)		M4V	12.23	13.37	?	19^h 20^m 48.0^s	−45° 33′ 30″	0.169 2351	19.2724
75	格利泽908 (Lalande 46650, BR Piscium)		M1V	8.98	10.12	3,653	23^h 49^m 12.5^s	+02° 24′ 04″	0.169 2163	19.2745
76	格利泽752 (Wolf 1055, HD 180617)	A	M2.5V	9.10	10.24	3,570	19^h 16^m 55.3^s	+05° 10′ 08″	0.169 0615	19.2922	拥有1个行星
76	格利泽752 (Wolf 1055, HD 180617)	B (VB 10)	M8V	17.45	18.59	2,600	19^h 16^m 57.6^s	+05° 09′ 02″	0.169 0615	19.2922	非常细小和暗淡的红矮星
77	葛利泽588 (CD-40 9712)		M2.5V	9.31	10.45	3,501	15^h 32^m 12.9^s	-41° 16′ 32″	0.168 9965	19.2996
78	王良三 (Gliese 34)	Achird (A)$	G3V	3.46#	4.60	5,937	00^h 49^m 06.3^s	+57° 48′ 55″	0.168 7186	19.3314
78	王良三 (Gliese 34)	B	K7V	7.51	8.65	?	00^h 49^m 06.3^s	+57° 48′ 55″	0.168 7186	19.3314
79	WISE 0350−5658§		Y1	22.47 J	23.70 J	?	03^h 50^m 00.3^s	-56° 58′ 30″	0.176 4^[29]	19.41
80	蛇夫座36 (Gliese 663)	Guniibuu (A)$	K1.5V	5.07#	6.20	5,103	17^h 15^m 20.9^s	-26° 36′ 09″	167.9617	19.4185
		B$	K1V	5.08#	6.21	5,199	17^h 15^m 21.0^s	-26° 36′ 10″
		C$	K5V	6.32#	7.45	4,561	17^h 16^m 13.4^s	-26° 32′ 46″
81	小犬座YZ (Ross 882, Gliese 285)		M4V	11.19	12.30	3,242	07^h 44^m 40.2^s	+03° 33′ 09″	0.166 9769	19.5330
82	WISE 1541-2250§		Y0.5	20.99 J	22.10 J	350	15^h 41^m 51.6^s	−22° 50′ 25″	0.166 9	19.54
83	格利泽1005 (Luyten 722-22, G 158-50)	A	M3.5V	11.60	12.71	3,227	00^h 15^m 28.1^s	-16° 08′ 02″	0.166 6^[30]	19.577
83	格利泽1005 (Luyten 722-22, G 158-50)	B	M V	14.02	15.13	?	00^h 15^m 28.1^s	-16° 08′ 02″	0.166 6^[30]	19.577
84	HR 7703 (279 G. Sagittarii, HD 191408, Gliese 783, IRAS 20079-3614)	A$	K2.5V	5.31#	6.41	4,974	20^h 11^m 11.93^s	–36° 06′ 04″	0.166 3272	19.609
84		B	M4V	11.50	12.60	?	20^h 11^m 11.93^s	–36° 06′ 04″	0.166 3272	19.609
85	天园增三 (e Eridani, Gliese 139, HD 20794)$		G8V	4.26#	5.35	5,401	03^h 19^m 55.7^s	−43° 04′ 11″	0.165 5242	19.7045	拥有3个行星
86	格利泽268 (Ross 986, QY Aurigae)	A	M4.5V	12.05	13.14	3,069	07^h 10^m 01.8^s	38° 31′ 46″	0.165 2147	19.7414
86	格利泽268 (Ross 986, QY Aurigae)	B	M V	12.45	13.54	?	07^h 10^m 01.8^s	38° 31′ 46″	0.165 2147	19.7414
87	孔雀六$		G8IV	3.55#	4.62	5,600	20^h 08^m 43.6^s	−66° 10′ 55″	0.163 9544	19.893
87	SIMP0136§		T2.5	13.25 J	14.32 J	?	01^h 36^m 56.5^s	+09° 33′ 47″	0.163 4478	19.955	流浪行星
#	系统	恒星	恒星类型	视星等	绝对星等	有效温度（±）（K）	赤经^[2]	赤纬^[2]	视差^[2]^[3]（±）（角秒）	距离^[4] （±）（光年）	附加参考资料及备注
#	名称		恒星类型	视星等	绝对星等	有效温度（±）（K）	历元J2000.0		视差^[2]^[3]（±）（角秒）	距离^[4] （±）（光年）	附加参考资料及备注

近距离恒星图

下图是距离太阳在14光年以内的32颗恒星位置图，双星和三合星会以实际的数量推叠，但真实的位置是以最靠近中心平面的那一颗为准，颜色则与上面的表相对应。

参考资料

^ Weaver, Harold F. The Visibility of Stars Without Optical Aid. Publications of the Astronomical Society of the Pacific. 1947, 59 (350): 232–243. Bibcode:1947PASP...59..232W. doi:10.1086/125956.
^ ^2.000 ^2.001 ^2.002 ^2.003 ^2.004 ^2.005 ^2.006 ^2.007 ^2.008 ^2.009 ^2.010 ^2.011 ^2.012 ^2.013 ^2.014 ^2.015 ^2.016 ^2.017 ^2.018 ^2.019 ^2.020 ^2.021 ^2.022 ^2.023 ^2.024 ^2.025 ^2.026 ^2.027 ^2.028 ^2.029 ^2.030 ^2.031 ^2.032 ^2.033 ^2.034 ^2.035 ^2.036 ^2.037 ^2.038 ^2.039 ^2.040 ^2.041 ^2.042 ^2.043 ^2.044 ^2.045 ^2.046 ^2.047 ^2.048 ^2.049 ^2.050 ^2.051 ^2.052 ^2.053 ^2.054 ^2.055 ^2.056 ^2.057 ^2.058 ^2.059 ^2.060 ^2.061 ^2.062 ^2.063 ^2.064 ^2.065 ^2.066 ^2.067 ^2.068 ^2.069 ^2.070 ^2.071 ^2.072 ^2.073 ^2.074 ^2.075 ^2.076 ^2.077 ^2.078 ^2.079 ^2.080 ^2.081 ^2.082 ^2.083 ^2.084 ^2.085 ^2.086 ^2.087 ^2.088 ^2.089 ^2.090 ^2.091 ^2.092 ^2.093 ^2.094 ^2.095 ^2.096 ^2.097 ^2.098 ^2.099 ^2.100 ^2.101 ^2.102 ^2.103 ^2.104 ^2.105 ^2.106 ^2.107 ^2.108 ^2.109 ^2.110 ^2.111 ^2.112 ^2.113 ^2.114 ^2.115 ^2.116 ^2.117 ^2.118 ^2.119 ^2.120 ^2.121 ^2.122 ^2.123 ^2.124 ^2.125 ^2.126 ^2.127 ^2.128 ^2.129 ^2.130 ^2.131 ^2.132 ^2.133 ^2.134 ^2.135 ^2.136 ^2.137 ^2.138 ^2.139 ^2.140 ^2.141 ^2.142 ^2.143 ^2.144 ^2.145 ^2.146 ^2.147 ^2.148 ^2.149 ^2.150 ^2.151 ^2.152 ^2.153 ^2.154 ^2.155 ^2.156 ^2.157 ^2.158 ^2.159 ^2.160 ^2.161 ^2.162 ^2.163 ^2.164 ^2.165 ^2.166 ^2.167 ^2.168 ^2.169 ^2.170 ^2.171 ^2.172 ^2.173 ^2.174 ^2.175 ^2.176 ^2.177 ^2.178 ^2.179 ^2.180 引用错误：没有为名为RECONS的参考文献提供内容
^ ^3.0 ^3.1 Parallaxes given by RECONS are a weighted mean of values in the sources given, as well as measurements by the RECONS program.
^ ^4.0 ^4.1 From parallax.
^ Sun Fact Sheet （页面存档备份，存于互联网档案馆）, NASA. Accessed on line 2007-11-08.
^ ^6.0 ^6.1 ^6.2 Kervella, Pierre; Thevenin, Frederic. A Family Portrait of the Alpha Centauri System: VLT Interferometer Studies the Nearest Stars. ESO Press Release 05/03 (ESO). 2003-03-15 [2007-11-08]. （原始内容存档于2008-06-16）.
^ ^7.00 ^7.01 ^7.02 ^7.03 ^7.04 ^7.05 ^7.06 ^7.07 ^7.08 ^7.09 ^7.10 ^7.11 ^7.12 ^7.13 ^7.14 ^7.15 ^7.16 ^7.17 ^7.18 ^7.19 ^7.20 ^7.21 ^7.22 ^7.23 ^7.24 ^7.25 ^7.26 ^7.27 ^7.28 ^7.29 ^7.30 ^7.31 ^7.32 ^7.33 ^7.34 ^7.35 ^7.36 ^7.37 ^7.38 ^7.39 ^7.40 ^7.41 ^7.42 General Catalogue of Trigonometric Parallaxes.
^ ^8.00 ^8.01 ^8.02 ^8.03 ^8.04 ^8.05 ^8.06 ^8.07 ^8.08 ^8.09 ^8.10 ^8.11 ^8.12 ^8.13 ^8.14 ^8.15 ^8.16 ^8.17 ^8.18 ^8.19 ^8.20 ^8.21 ^8.22 ^8.23 ^8.24 ^8.25 ^8.26 ^8.27 ^8.28 Hipparcos Catalogue.
^ Burgasser et al. 2000
^ ^10.0 ^10.1 ^10.2 Visual binary orbits and masses post Hipparcos （页面存档备份，存于互联网档案馆）, Staffan Söderhjelm, Astronomy and Astrophysics 341(January 1999),pp. 121–140.
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^ Luhman, K. L. Discovery of a Binary Brown Dwarf at 2 Parsecs from the Sun (PDF). Astrophysical Journal Letters（to be published）. ^{[失效链接]}
^ Davy Kirkpatrick, J.; Gelino, Christopher R.; Faherty, Jacqueline K.; Meisner, Aaron M.; Caselden, Dan; Schneider, Adam C.; Marocco, Federico; Cayago, Alfred J.; Smart, R. L.; Eisenhardt, Peter R.; Kuchner, Marc J.; Wright, Edward L.; Cushing, Michael C.; Allers, Katelyn N.; Bardalez Gagliuffi, Daniella C.; Burgasser, Adam J.; Gagne, Jonathan; Logsdon, Sarah E.; Martin, Emily C.; Ingalls, James G.; Lowrance, Patrick J.; Abrahams, Ellianna S.; Aganze, Christian; Gerasimov, Roman; Gonzales, Eileen C.; Hsu, Chih-Chun; Kamraj, Nikita; Kiman, Rocio; Rees, Jon; et al. The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs. The Astrophysical Journal Supplement Series. 2021, 253 (1): 7. Bibcode:2021ApJS..253....7K. S2CID 227126954. arXiv:2011.11616  . doi:10.3847/1538-4365/abd107.
^ Ya. V. Pavlenko, H. R. A. Jones, Yu. Lyubchik, J. Tennyson, and D. J. Pinfield. Spectral energy distribution for GJ406. Astronomy and Astrophysics. February 2006, 447 (2): 709–717 [2020-09-20]. doi:10.1051/0004-6361:20052979. （原始内容存档于2019-06-14）.
^ Carbon monoxide bands in M dwarfs （页面存档备份，存于互联网档案馆）, Y. V. Pavlenko and H. R. A. Jones, Astronomy and Astrophysics 396(December 2002),pp. 967–975. doi:10.1051/0004-6361:20021454
^ Table 2, The physical properties of normal A stars （页面存档备份，存于互联网档案馆）, Saul J. Adelman, pp. 1–11, The A-Star Puzzle, Proceedings of the International Astronomical Union, edited by J. Zverko, J. Ziznovsky, S. J. Adelman, and W. W. Weiss, Cambridge, UK: Cambridge University Press, 2004. doi:10.1017/S1743921304004314
^ Adopted value, The Age and Progenitor Mass of Sirius B （页面存档备份，存于互联网档案馆）, James Liebert, Patrick A. Young, David Arnett, J.B. Holberg, and Kurtis A. Williams, The Astrophysical Journal 630, #1(September 2005),pp. L69–L72.
^ ^18.0 ^18.1 Kirkpatrick, J. Davy; Michael C. Cushing; Christopher R. Gelino; Roger L. Griffith; Michael F. Skrutskie; Kenneth A. Marsh; Edward L. Wright; Amanda K. Mainzer; Peter R. Eisenhardt; Ian S. McLean; Maggie A. Thompson; James M. Bauer; Dominic J. Benford; Carrie R. Bridge; Sean E. Lake; Sara M. Petty; S. Adam Stanford; Chao-Wei Tsai; Vanessa Bailey; Charles A. Beichman; John J. Bochanski; Adam J. Burgasser; Peter L. Capak; Kelle L. Cruz; Philip M. Hinz; Jeyhan S. Kartaltepe; Russell P. Knox; Swarnima Manohar; Daniel Masters; Maria Morales-Calderon; Lisa A. Prato; Timothy J. Rodigas; Mara Salvato; Steven D. Schurr; Nicholas Z. Scoville; Robert A. Simcoe; Karl R. Stapelfeldt; Daniel Stern; Nathan D. Stock; William D. Vacca. The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer(WISE). 2011. arXiv:1108.4677v1  [astro-ph.SR]. cite arXiv模板填写了不支持的参数 (帮助)
^ ^19.0 ^19.1 ^19.2 ^19.3 ^19.4 ^19.5 Systems with their first accurate trigonometric parallaxes measured by RECONS
^ The solar neighborhood IV: discovery of the twentieth nearest star （页面存档备份，存于互联网档案馆）, Todd J. Henry, Philip A. Ianna, J. Davy Kirkpatrick, Hartmut Jahreiss, The Astronomical Journal 114, #1(July 1997),pp. 388–395. doi:10.1086/118482
^ ^21.0 ^21.1 ^21.2 ^21.3 The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample （页面存档备份，存于互联网档案馆）, Todd J. Henry, Wei-Chun Jao, John P. Subasavage, Thomas D. Beaulieu, Philip A. Ianna, Edgardo Costa, René A. Méndez, The Astronomical Journal 132, #6(December 2006),pp. 2360–2371. doi:10.1086/508233
^ ^22.0 ^22.1 The very nearby M/T dwarf binary SCR 1845-6357 （页面存档备份，存于互联网档案馆）, Markus Kasper, Beth A. Biller, Adam Burrows, Wolfgang Brandner, Jano Budaj, and Laird M. Close, Astronomy and Astrophysics 471, #2(August 2007),pp. 655–659. doi:10.1051/0004-6361:20077881
^ The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with μ >= 1.0" yr^-1 (Motion sample) （页面存档备份，存于互联网档案馆）, Wei-Chun Jao, Todd J. Henry, John P. Subasavage, Misty A. Brown, Philip A. Ianna, Jennifer L. Bartlett, Edgardo Costa, René A. Méndez, The Astronomical Journal 129, #4(April 2005),pp. 1954–1967. doi:10.1086/428489
^ ^24.0 ^24.1 The Solar Neighborhood. XIV. Parallaxes from the Cerro Tololo Inter-American Observatory Parallax Investigation—First Results from the 1.5 m Telescope Program （页面存档备份，存于互联网档案馆）, Edgardo Costa, René A. Méndez, W.-C. Jao, Todd J. Henry, John P. Subasavage, Misty A. Brown, Philip A. Ianna, and Jennifer Bartlett, The Astronomical Journal 130, #1(July 2005),pp. 337–349. doi:10.1086/430473
^ Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; et al. Gaia Data Release 2. Summary of the contents and survey properties. Astronomy & Astrophysics. 2018. Bibcode:2018A&A...616A...1G. arXiv:1804.09365  . doi:10.1051/0004-6361/201833051.
^ van Leeuwen, F., Validation of the new Hipparcos reduction, Astronomy and Astrophysics, November 2007, 474 (2): 653–664, Bibcode:2007A&A...474..653V, S2CID 18759600, arXiv:0708.1752  , doi:10.1051/0004-6361:20078357
^ Burgasser, Adam J.; Tinney, C. G.; Cushing, Michael C.; Saumon, Didier; Marley, Mark S.; Bennett, Clara S.; Kirkpatrick, J. Davy. 2MASS J09393548-2448279: The Coldest and Least Luminous Brown Dwarf Binary Known? (PDF). The Astrophysical Journal. 2008, 689 (1): L53–L56 [2023-03-20]. Bibcode:2008ApJ...689L..53B. doi:10.1086/595747  . （原始内容存档 (PDF)于2022-01-28）.
^ ^28.0 ^28.1 Dupuy, Trent J.; Liu, Michael C. The Hawaii Infrared Parallax Program. I. Ultracool Binaries and the L/T Transition. The Astrophysical Journal Supplement. 2012, 201 (2): 19. Bibcode:2012ApJS..201...19D. S2CID 119256363. arXiv:1201.2465  . doi:10.1088/0067-0049/201/2/19.
^ Kirkpatrick, J. Davy; Gelino, Christopher R.; Faherty, Jacqueline K.; Meisner, Aaron M.; Caselden, Dan; Schneider, Adam C.; Marocco, Federico; Cayago, Alfred J.; Smart, R. L.; Eisenhardt, Peter R.; Kuchner, Marc J. The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs. The Astrophysical Journal Supplement Series. 2021, 253 (1): 7. Bibcode:2021ApJS..253....7K. S2CID 227126954. arXiv:2011.11616  . doi:10.3847/1538-4365/abd107.
^ Benedict, G. F.; Henry, T. J.; Franz, O. G.; McArthur, B. E.; Wasserman, L. H.; Jao, Wei-Chun; Cargile, P. A.; Dieterich, S. B.; Bradley, A. J.; Nelan, E. P.; Whipple, A. L. The Solar Neighborhood. XXXVII. The Mass–Luminosity Relation for Main-Sequence M Dwarfs. The Astronomical Journal. 2016, 152 (5): 141. Bibcode:2016AJ....152..141B. S2CID 54029447. arXiv:1608.04775  . doi:10.3847/0004-6256/152/5/141.

外部链接

"The 100 nearest star systems" （页面存档备份，存于互联网档案馆）, Research Consortium on Nearby Stars
NStars database. Northern Arizona University. [2005-10-24]. （原始内容存档于2005-10-30）.
Nemiroff, R.; Bonnell, J. (编). Map of the 25 nearest star systems. Astronomy Picture of the Day. NASA. March 18, 2001 [2005-10-24].
Notable Nearby Stars. SolStation. [2005-10-24]. （原始内容存档于2016-03-21）.
Cool stars in the solar Neighbourhood. D. Montes, UCM. [2005-11-14]. （原始内容存档于2012-09-29）.
The dynamics of the closest stars （页面存档备份，存于互联网档案馆）
Takeda, G.; E. B. Ford; A. Sills; F. A. Rasio; D. A. Fischer; J. A. Valenti. Structure and Evolution of Nearby Stars with Planets II. Physical Properties of ~ 1000 Cool Stars from the SPOCS Catalog. California & Carnegie Planet Search. 2006 [2006-10-13]. （原始内容存档于2016-03-03）.
Nearest Stars 3D View （页面存档备份，存于互联网档案馆）
Table 4 "The Census of Stars and Brown Dwarfs within 8 Parsecs of the Sun" in Kirkpatrick et al. (2012) Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function, http://arxiv.org/pdf/1205.2122v1.pdf （页面存档备份，存于互联网档案馆）
http://phl.upr.edu/projects/nearby-stars-catalog （页面存档备份，存于互联网档案馆）

[1] Weaver, Harold F. The Visibility of Stars Without Optical Aid. Publications of the Astronomical Society of the Pacific. 1947, 59 (350): 232–243. Bibcode:1947PASP...59..232W. doi:10.1086/125956.

[RECONS-2] 2.000 ^2.001 ^2.002 ^2.003 ^2.004 ^2.005 ^2.006 ^2.007 ^2.008 ^2.009 ^2.010 ^2.011 ^2.012 ^2.013 ^2.014 ^2.015 ^2.016 ^2.017 ^2.018 ^2.019 ^2.020 ^2.021 ^2.022 ^2.023 ^2.024 ^2.025 ^2.026 ^2.027 ^2.028 ^2.029 ^2.030 ^2.031 ^2.032 ^2.033 ^2.034 ^2.035 ^2.036 ^2.037 ^2.038 ^2.039 ^2.040 ^2.041 ^2.042 ^2.043 ^2.044 ^2.045 ^2.046 ^2.047 ^2.048 ^2.049 ^2.050 ^2.051 ^2.052 ^2.053 ^2.054 ^2.055 ^2.056 ^2.057 ^2.058 ^2.059 ^2.060 ^2.061 ^2.062 ^2.063 ^2.064 ^2.065 ^2.066 ^2.067 ^2.068 ^2.069 ^2.070 ^2.071 ^2.072 ^2.073 ^2.074 ^2.075 ^2.076 ^2.077 ^2.078 ^2.079 ^2.080 ^2.081 ^2.082 ^2.083 ^2.084 ^2.085 ^2.086 ^2.087 ^2.088 ^2.089 ^2.090 ^2.091 ^2.092 ^2.093 ^2.094 ^2.095 ^2.096 ^2.097 ^2.098 ^2.099 ^2.100 ^2.101 ^2.102 ^2.103 ^2.104 ^2.105 ^2.106 ^2.107 ^2.108 ^2.109 ^2.110 ^2.111 ^2.112 ^2.113 ^2.114 ^2.115 ^2.116 ^2.117 ^2.118 ^2.119 ^2.120 ^2.121 ^2.122 ^2.123 ^2.124 ^2.125 ^2.126 ^2.127 ^2.128 ^2.129 ^2.130 ^2.131 ^2.132 ^2.133 ^2.134 ^2.135 ^2.136 ^2.137 ^2.138 ^2.139 ^2.140 ^2.141 ^2.142 ^2.143 ^2.144 ^2.145 ^2.146 ^2.147 ^2.148 ^2.149 ^2.150 ^2.151 ^2.152 ^2.153 ^2.154 ^2.155 ^2.156 ^2.157 ^2.158 ^2.159 ^2.160 ^2.161 ^2.162 ^2.163 ^2.164 ^2.165 ^2.166 ^2.167 ^2.168 ^2.169 ^2.170 ^2.171 ^2.172 ^2.173 ^2.174 ^2.175 ^2.176 ^2.177 ^2.178 ^2.179 ^2.180 引用错误：没有为名为RECONS的参考文献提供内容

[plxfn-3] 3.0 ^3.1 Parallaxes given by RECONS are a weighted mean of values in the sources given, as well as measurements by the RECONS program.

[distfn-4] 4.0 ^4.1 From parallax.

[5] Sun Fact Sheet （页面存档备份，存于互联网档案馆）, NASA. Accessed on line 2007-11-08.

[ESO2003-6] 6.0 ^6.1 ^6.2 Kervella, Pierre; Thevenin, Frederic. A Family Portrait of the Alpha Centauri System: VLT Interferometer Studies the Nearest Stars. ESO Press Release 05/03 (ESO). 2003-03-15 [2007-11-08]. （原始内容存档于2008-06-16）.

[Y-7] 7.00 ^7.01 ^7.02 ^7.03 ^7.04 ^7.05 ^7.06 ^7.07 ^7.08 ^7.09 ^7.10 ^7.11 ^7.12 ^7.13 ^7.14 ^7.15 ^7.16 ^7.17 ^7.18 ^7.19 ^7.20 ^7.21 ^7.22 ^7.23 ^7.24 ^7.25 ^7.26 ^7.27 ^7.28 ^7.29 ^7.30 ^7.31 ^7.32 ^7.33 ^7.34 ^7.35 ^7.36 ^7.37 ^7.38 ^7.39 ^7.40 ^7.41 ^7.42 General Catalogue of Trigonometric Parallaxes.

[H-8] 8.00 ^8.01 ^8.02 ^8.03 ^8.04 ^8.05 ^8.06 ^8.07 ^8.08 ^8.09 ^8.10 ^8.11 ^8.12 ^8.13 ^8.14 ^8.15 ^8.16 ^8.17 ^8.18 ^8.19 ^8.20 ^8.21 ^8.22 ^8.23 ^8.24 ^8.25 ^8.26 ^8.27 ^8.28 Hipparcos Catalogue.

[B-9] Burgasser et al. 2000

[S-10] 10.0 ^10.1 ^10.2 Visual binary orbits and masses post Hipparcos （页面存档备份，存于互联网档案馆）, Staffan Söderhjelm, Astronomy and Astrophysics 341(January 1999),pp. 121–140.

[11] Barnard's Star and the M Dwarf Temperature Scale （页面存档备份，存于互联网档案馆）, P. C. Dawson and M. M. de Robertis, The Astronomical Journal 127, #5(May 2004),pp. 2909–2914. doi:10.1086/383289

[12] Luhman, K. L. Discovery of a Binary Brown Dwarf at 2 Parsecs from the Sun (PDF). Astrophysical Journal Letters（to be published）. ^{[失效链接]}

[Kirkpatrick2021-13] Davy Kirkpatrick, J.; Gelino, Christopher R.; Faherty, Jacqueline K.; Meisner, Aaron M.; Caselden, Dan; Schneider, Adam C.; Marocco, Federico; Cayago, Alfred J.; Smart, R. L.; Eisenhardt, Peter R.; Kuchner, Marc J.; Wright, Edward L.; Cushing, Michael C.; Allers, Katelyn N.; Bardalez Gagliuffi, Daniella C.; Burgasser, Adam J.; Gagne, Jonathan; Logsdon, Sarah E.; Martin, Emily C.; Ingalls, James G.; Lowrance, Patrick J.; Abrahams, Ellianna S.; Aganze, Christian; Gerasimov, Roman; Gonzales, Eileen C.; Hsu, Chih-Chun; Kamraj, Nikita; Kiman, Rocio; Rees, Jon; et al. The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs. The Astrophysical Journal Supplement Series. 2021, 253 (1): 7. Bibcode:2021ApJS..253....7K. S2CID 227126954. arXiv:2011.11616  . doi:10.3847/1538-4365/abd107.

[aaa447-14] Ya. V. Pavlenko, H. R. A. Jones, Yu. Lyubchik, J. Tennyson, and D. J. Pinfield. Spectral energy distribution for GJ406. Astronomy and Astrophysics. February 2006, 447 (2): 709–717 [2020-09-20]. doi:10.1051/0004-6361:20052979. （原始内容存档于2019-06-14）.

[15] Carbon monoxide bands in M dwarfs （页面存档备份，存于互联网档案馆）, Y. V. Pavlenko and H. R. A. Jones, Astronomy and Astrophysics 396(December 2002),pp. 967–975. doi:10.1051/0004-6361:20021454

[16] Table 2, The physical properties of normal A stars （页面存档备份，存于互联网档案馆）, Saul J. Adelman, pp. 1–11, The A-Star Puzzle, Proceedings of the International Astronomical Union, edited by J. Zverko, J. Ziznovsky, S. J. Adelman, and W. W. Weiss, Cambridge, UK: Cambridge University Press, 2004. doi:10.1017/S1743921304004314

[17] Adopted value, The Age and Progenitor Mass of Sirius B （页面存档备份，存于互联网档案馆）, James Liebert, Patrick A. Young, David Arnett, J.B. Holberg, and Kurtis A. Williams, The Astrophysical Journal 630, #1(September 2005),pp. L69–L72.

[Kirkpatrick2011v1-18] 18.0 ^18.1 Kirkpatrick, J. Davy; Michael C. Cushing; Christopher R. Gelino; Roger L. Griffith; Michael F. Skrutskie; Kenneth A. Marsh; Edward L. Wright; Amanda K. Mainzer; Peter R. Eisenhardt; Ian S. McLean; Maggie A. Thompson; James M. Bauer; Dominic J. Benford; Carrie R. Bridge; Sean E. Lake; Sara M. Petty; S. Adam Stanford; Chao-Wei Tsai; Vanessa Bailey; Charles A. Beichman; John J. Bochanski; Adam J. Burgasser; Peter L. Capak; Kelle L. Cruz; Philip M. Hinz; Jeyhan S. Kartaltepe; Russell P. Knox; Swarnima Manohar; Daniel Masters; Maria Morales-Calderon; Lisa A. Prato; Timothy J. Rodigas; Mara Salvato; Steven D. Schurr; Nicholas Z. Scoville; Robert A. Simcoe; Karl R. Stapelfeldt; Daniel Stern; Nathan D. Stock; William D. Vacca. The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer(WISE). 2011. arXiv:1108.4677v1  [astro-ph.SR]. cite arXiv模板填写了不支持的参数 (帮助)

[recent-19] 19.0 ^19.1 ^19.2 ^19.3 ^19.4 ^19.5 Systems with their first accurate trigonometric parallaxes measured by RECONS

[henry1997-20] The solar neighborhood IV: discovery of the twentieth nearest star （页面存档备份，存于互联网档案馆）, Todd J. Henry, Philip A. Ianna, J. Davy Kirkpatrick, Hartmut Jahreiss, The Astronomical Journal 114, #1(July 1997),pp. 388–395. doi:10.1086/118482

[henry2006-21] 21.0 ^21.1 ^21.2 ^21.3 The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample （页面存档备份，存于互联网档案馆）, Todd J. Henry, Wei-Chun Jao, John P. Subasavage, Thomas D. Beaulieu, Philip A. Ianna, Edgardo Costa, René A. Méndez, The Astronomical Journal 132, #6(December 2006),pp. 2360–2371. doi:10.1086/508233

[nearmt-22] 22.0 ^22.1 The very nearby M/T dwarf binary SCR 1845-6357 （页面存档备份，存于互联网档案馆）, Markus Kasper, Beth A. Biller, Adam Burrows, Wolfgang Brandner, Jano Budaj, and Laird M. Close, Astronomy and Astrophysics 471, #2(August 2007),pp. 655–659. doi:10.1051/0004-6361:20077881

[23] The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with μ >= 1.0" yr^-1 (Motion sample) （页面存档备份，存于互联网档案馆）, Wei-Chun Jao, Todd J. Henry, John P. Subasavage, Misty A. Brown, Philip A. Ianna, Jennifer L. Bartlett, Edgardo Costa, René A. Méndez, The Astronomical Journal 129, #4(April 2005),pp. 1954–1967. doi:10.1086/428489

[costa2005-24] 24.0 ^24.1 The Solar Neighborhood. XIV. Parallaxes from the Cerro Tololo Inter-American Observatory Parallax Investigation—First Results from the 1.5 m Telescope Program （页面存档备份，存于互联网档案馆）, Edgardo Costa, René A. Méndez, W.-C. Jao, Todd J. Henry, John P. Subasavage, Misty A. Brown, Philip A. Ianna, and Jennifer Bartlett, The Astronomical Journal 130, #1(July 2005),pp. 337–349. doi:10.1086/430473

[GaiaDR2-25] Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; et al. Gaia Data Release 2. Summary of the contents and survey properties. Astronomy & Astrophysics. 2018. Bibcode:2018A&A...616A...1G. arXiv:1804.09365  . doi:10.1051/0004-6361/201833051.

[aaa474_2_653-26] van Leeuwen, F., Validation of the new Hipparcos reduction, Astronomy and Astrophysics, November 2007, 474 (2): 653–664, Bibcode:2007A&A...474..653V, S2CID 18759600, arXiv:0708.1752  , doi:10.1051/0004-6361:20078357

[Burgasser2008-27] Burgasser, Adam J.; Tinney, C. G.; Cushing, Michael C.; Saumon, Didier; Marley, Mark S.; Bennett, Clara S.; Kirkpatrick, J. Davy. 2MASS J09393548-2448279: The Coldest and Least Luminous Brown Dwarf Binary Known? (PDF). The Astrophysical Journal. 2008, 689 (1): L53–L56 [2023-03-20]. Bibcode:2008ApJ...689L..53B. doi:10.1086/595747  . （原始内容存档 (PDF)于2022-01-28）.

[Dupuy_&_Liu2012-28] 28.0 ^28.1 Dupuy, Trent J.; Liu, Michael C. The Hawaii Infrared Parallax Program. I. Ultracool Binaries and the L/T Transition. The Astrophysical Journal Supplement. 2012, 201 (2): 19. Bibcode:2012ApJS..201...19D. S2CID 119256363. arXiv:1201.2465  . doi:10.1088/0067-0049/201/2/19.

[:0-29] Kirkpatrick, J. Davy; Gelino, Christopher R.; Faherty, Jacqueline K.; Meisner, Aaron M.; Caselden, Dan; Schneider, Adam C.; Marocco, Federico; Cayago, Alfred J.; Smart, R. L.; Eisenhardt, Peter R.; Kuchner, Marc J. The Field Substellar Mass Function Based on the Full-sky 20 pc Census of 525 L, T, and Y Dwarfs. The Astrophysical Journal Supplement Series. 2021, 253 (1): 7. Bibcode:2021ApJS..253....7K. S2CID 227126954. arXiv:2011.11616  . doi:10.3847/1538-4365/abd107.

[Benedict-30] Benedict, G. F.; Henry, T. J.; Franz, O. G.; McArthur, B. E.; Wasserman, L. H.; Jao, Wei-Chun; Cargile, P. A.; Dieterich, S. B.; Bradley, A. J.; Nelan, E. P.; Whipple, A. L. The Solar Neighborhood. XXXVII. The Mass–Luminosity Relation for Main-Sequence M Dwarfs. The Astronomical Journal. 2016, 152 (5): 141. Bibcode:2016AJ....152..141B. S2CID 54029447. arXiv:1608.04775  . doi:10.3847/0004-6256/152/5/141.

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