金牛座V773
金牛座V773是在黄道星座金牛座的年轻聚星，位于它的中心区域[7]。这是一颗金牛T星型变星，其视星等范围从10.59到10.95[4]，它太黯淡了，因此肉眼看不见。根据各种估计，该系统距离太阳约433光年。它位于林兹1495（Lynds 1495）暗星云的附近[7]。
| 观测资料 历元 J2000 | |
|---|---|
| 星座 | 金牛座 |
| 星官 | |
| 赤经 | 04h 14m 12.926s[3] |
| 赤纬 | 28° 12′ 12.36″[3] |
| 视星等（V） | 10.59 to 10.95[4] |
| 特性 | |
| 光谱分类 | K3Ve (Li)[5] |
| 变星类型 | 猎户型变星 + BY Dra[4] |
| 天体测定 | |
| 自行 (μ) | 赤经：6.540 mas/yr 赤纬：−27.792 mas/yr |
| 视差 (π) | 8.3261 ± 0.1313 mas |
| 距离 | 433.1 ± 7.5 ly (132.8+2.3 − pc) |
| 轨道[2] | |
| 主星 | 金牛座V773 AB |
| 伴星 | 金牛座V773 C |
| 绕行周期 (P) | 624+83 −52 yr |
| 半长轴 (a) | 1,013+93 −74 mas |
| 偏心率 (e) | 0.40+0.04 −0.05 |
| 倾斜角 (i) | 97.3+0.6 −° |
| 升交点黄经 (Ω) | 104.6+1.3 −° |
| 近心点 历元 (T) | 1,740+26 −40 |
| 近心点幅角 (ω) (secondary) | 107.8+4.5 −° |
| 轨道[2] | |
| 主星 | 金牛座V773 A |
| 伴星 | 金牛座V773 B |
| 绕行周期 (P) | 26.50+0.07 − yr |
| 半长轴 (a) | 117.7±0.86 mas |
| 偏心率 (e) | 0.104+0.009 − |
| 倾斜角 (i) | 69.25+0.40 −° |
| 升交点黄经 (Ω) | 290.54+0.40 −° |
| 近心点 历元 (T) | 2,010.11+0.12 − |
| 近心点幅角 (ω) (secondary) | 266.0+1.5 −° |
| 半振幅 (K1) (primary) | 6.50+0.50 −[6] km/s |
| 轨道[7] | |
| 主星 | 金牛座V773 Aa |
| 伴星 | 金牛座V773 Ab |
| 绕行周期 (P) | 51.1033±0.0018 d |
| 半长轴 (a) | 2.809±0.033 mas |
| 偏心率 (e) | 0.2713+0.0066 − |
| 倾斜角 (i) | 68.5+1.6 −° |
| 升交点黄经 (Ω) | 62.4+1.1 −° |
| 近心点 历元 (T) | 53,059.75±0.28 MJD |
| 近心点幅角 (ω) (secondary) | 5.6+2.2 −° |
| 半振幅 (K1) (primary) | 35.72+0.46 − km/s |
| 半振幅 (K2) (secondary) | 42.9+1.3 − km/s |
| 详细资料 | |
| Aa | |
| 质量 | 1.55+0.11 −[7] M☉ |
| 半径 | 2.22[8] R☉ |
| 表面重力 (log g) | 3.93[8] |
| 亮度 | 2.56[8] L☉ |
| 温度 | 4,900[8] K |
| 年龄 | 3+1 −[2] Myr |
| Ab | |
| 质量 | 1.293+0.068 −[7] M☉ |
| 半径 | 1.74[8] R☉ |
| 表面重力 (log g) | 4.08[8] |
| 亮度 | 1.37[8] L☉ |
| 温度 | 4,740[8] K |
| 其他命名 | |
| 参考数据库 | |
| SIMBAD | 资料 |
| Aa | |||||||||||||||
| Period = 51.1 d | |||||||||||||||
| Ab | |||||||||||||||
| Period = 26.5 yr | |||||||||||||||
| B(ab) | |||||||||||||||
| Period = 624 yr | |||||||||||||||
| C | |||||||||||||||
这个系统在1974年被吕德格伦（a.E.Rydgren）及其同事确认为金牛T星[10]。1983年，从这个来源探测到无线电发射[11]。在1993年，它被发现是一颗双星，角距离约为150 mas：这两个成员被指定为A和B。成员A被发现是具有51天轨道周期的双线光谱联星。在2003年，发现该系统的第三颗成员，成员C[7]，与成员A的角距离为256 mas。
A–B对的轨道解为B成员提供了出乎意料的高动态质量2.69±0.67 太阳质量，这表明它也可能是一个联星系统[6]。一颗质量如此之大的恒星光度是太阳的17倍，这与观测到的光学光度不一致。对成员B的光度测定表明，它正沿着视线从尘埃中经历消光。该成员在K波段是可变的，这与轨道上的尘埃团或云一致[2]。
2010年，在金牛座V773系统中观测到了一次扩展的星食。这被解释为成员B的环双星盘从成员A的前面经过。星食遮蔽了成员A 70%的发射，并持续了150天[2]。
参考资料
编辑- ^ MAST: Barbara A. Mikulski Archive for Space Telescopes, Space Telescope Science Institute, [8 December 2021], （原始内容存档于2023-03-27）.
- ^ 2.0 2.1 2.2 2.3 2.4 2.5 Kenworthy, M. A.; et al, Eclipse of the V773 Tau B circumbinary disc, Astronomy & Astrophysics, October 2022, 666: A61, Bibcode:2022A&A...666A..61K, S2CID 250451004, arXiv:2207.05575
, doi:10.1051/0004-6361/202243441, A61.
- ^ 3.0 3.1 Brown, A. G. A.; et al. Gaia Early Data Release 3: Summary of the contents and survey properties. Astronomy & Astrophysics. 2021, 649: A1. Bibcode:2021A&A...649A...1G. S2CID 227254300. arXiv:2012.01533 . doi:10.1051/0004-6361/202039657 . 已忽略未知参数
|collaboration=(帮助) (勘误: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR. - ^ 4.0 4.1 4.2 Samus, N. N.; et al, General Catalogue of Variable Stars, Astronomy Reports, 5.1, 2017, 61 (1): 80–88, Bibcode:2017ARep...61...80S, S2CID 125853869, doi:10.1134/S1063772917010085.
- ^ Herbig, G. H., Radial velocities and spectral types of T Tauri stars, Astrophysical Journal, 1977, 214: 747–758, Bibcode:1977ApJ...214..747H, doi:10.1086/155304 .
- ^ 6.0 6.1 Boden, Andrew F.; et al, A Surprising Dynamical Mass for V773 Tau B, The Astrophysical Journal, March 2012, 747 (1): 17, Bibcode:2012ApJ...747...17B, S2CID 118997621, arXiv:1112.1018 , doi:10.1088/0004-637X/747/1/17, 17.
- ^ 7.0 7.1 7.2 7.3 7.4 7.5 Torres, Rosa M.; et al, VLBA Determination of the Distance to nearby Star-forming Regions. V. Dynamical Mass, Distance, and Radio Structure of V773 Tau A, The Astrophysical Journal, March 2012, 747 (1): 18, Bibcode:2012ApJ...747...18T, S2CID 494696, arXiv:1112.0114 , doi:10.1088/0004-637X/747/1/18, 18.
- ^ 8.0 8.1 8.2 8.3 8.4 8.5 8.6 8.7 Boden, Andrew F.; et al, Dynamical Masses for Pre-Main-Sequence Stars: A Preliminary Physical Orbit for V773 Tau A, The Astrophysical Journal, December 2007, 670 (2): 1214–1224, Bibcode:2007ApJ...670.1214B, S2CID 40241514, arXiv:0706.2376 , doi:10.1086/521296.
- ^ HD 283447. SIMBAD. 斯特拉斯堡天文资料中心.
- ^ Rydgren, A. E.; et al, The nature of the objects of Joy: a study of the T Tauri phenomenon., Astrophysical Journal Supplement Series, March 1976, 30: 307–336, Bibcode:1976ApJS...30..307R, doi:10.1086/190364. See notes about HD 283447.
- ^ Kutner, M. L.; et al, Detection of 6 CM radio emission from late-type PMS stars with weak chromospheric emission, Astronomical Journal, October 1986, 92: 895–897, Bibcode:1986AJ.....92..895K, doi:10.1086/114223 .
进阶读物
编辑- Umemoto, T.; et al, Hagiwara, Yoshiaki; et al , 编, Detection of a Radio Flare at Millimeter-Wavelengths from the X-ray T Tauri Star V773 Tau, Approaching Micro-Arcsecond Resolution with VSOP-2, proceedings of the conference held 3–7 December 2007, at ISAS/JAXA, Sagamihara, Kanagawa, Japan, Astrophysics and Technologies ASP Conference Series 402, August 2009, 402: 400, Bibcode:2009ASPC..402..400U.
- Massi, M.; et al, Interacting coronae of two T Tauri stars: first observational evidence for solar-like helmet streamers, Astronomy and Astrophysics, March 2008, 480 (2): 489–494, Bibcode:2008A&A...480..489M, S2CID 11380885, arXiv:0712.0718 , doi:10.1051/0004-6361:20078637.
- Massi, M.; et al, Synchrotron emission from the T Tauri binary system V773 Tauri A, Astronomy and Astrophysics, July 2006, 453 (3): 959–964, Bibcode:2006A&A...453..959M, S2CID 14134438, arXiv:astro-ph/0604124 , doi:10.1051/0004-6361:20053535.
- Duchêne, G.; et al, No Fossil Disk in the T Tauri Multiple System V773 Tauri, The Astrophysical Journal, July 2003, 592 (1): 288–298, Bibcode:2003ApJ...592..288D, S2CID 119094313, arXiv:astro-ph/0303648 , doi:10.1086/375624.
- Tamazian, Vakhtang S.; et al, Preliminary Orbits and System Masses for Five Binary T Tauri Stars, The Astrophysical Journal, October 2002, 578 (2): 925–934, Bibcode:2002ApJ...578..925T, S2CID 123360722, doi:10.1086/342621.
- Massi, M.; et al, Periodic radio flaring on the T Tauri star V 773 Tauri, Astronomy and Astrophysics, January 2002, 382: 152–156, Bibcode:2002A&A...382..152M, S2CID 56413068, doi:10.1051/0004-6361:20011585.
- Tsuboi, Yohko; et al, ASCA Detection of a Superhot 100 Million K X-Ray Flare on the Weak-Lined T Tauri Star V773 Tauri, The Astrophysical Journal, August 1998, 503 (2): 894–901, Bibcode:1998ApJ...503..894T, S2CID 121483342, doi:10.1086/306024 .
- Skinner, Stephen L.; et al, ASCA Observations of the Barnard 209 Dark Cloud and an Intense X-Ray Flare on V773 Tauri, The Astrophysical Journal, September 1997, 486 (2): 886–902, Bibcode:1997ApJ...486..886S, S2CID 123108722, doi:10.1086/304561, hdl:2060/19980076126 .
- Skinner, S. L., Time-Resolved X-ray Spectroscopy of the Weak-lined T Tauri Star V773 Tau, Bulletin of the American Astronomical Society, May 1996, 28: 884, Bibcode:1996AAS...188.4008S.
- Welty, Alan D., Discovery of a Pre-Main-Sequence Spectrscopic Binary: V773 Tauri, Astronomical Journal, August 1995, 110: 776, Bibcode:1995AJ....110..776W, doi:10.1086/117562.