军井一
军井一（Iota Leporis，ι Leporis）是在南天星座天兔座的一颗三合星[5]系统。它的视星等为4.45等，肉眼可见，它是蓝白光的点光源[3]。基于从地球量测的每年14.07mas的视差[2]，该系统位于距离太阳大约232光年之处
| 观测资料 历元 J2000.0 | |
|---|---|
| 星座 | 天兔座 |
| 星官 | 军井（参宿） |
| 赤经 | 05h 12m 17.90190s[2] |
| 赤纬 | −11° 52′ 09.1863″[2] |
| 视星等（V） | 4.45[3] |
| 特性 | |
| 光谱分类 | B7.5 Vn[4] + K7.2 XR? + G8 Ve[5] |
| U−B 色指数 | −0.40[3] |
| B−V 色指数 | −0.10[3] |
| 天体测定 | |
| 径向速度 (Rv) | +23.50[6] km/s |
| 自行 (μ) | 赤经：+24.39[2] mas/yr 赤纬：−31.02[2] mas/yr |
| 视差 (π) | 14.07 ± 0.16[2] mas |
| 距离 | 232 ± 3 ly (71.1 ± 0.8 pc) |
| 绝对星等 (MV) | 0.01[7] |
| 详细资料 | |
| 军井一A（ι Lep A） | |
| 质量 | 3.37±0.02[8] M☉ |
| 表面重力 (log g) | 4.25[9] |
| 亮度 | 153[8] L☉ |
| 温度 | 13,781±469[9] K |
| 自转速度 (v sin i) | 185[9] km/s |
| 年龄 | 94[7] Myr |
| 其他命名 | |
| 参考数据库 | |
| SIMBAD | 资料 |
主星A是一颗B型主序星，恒星分类为B7.5Vn[4]，此处尾码的“n”表示有自转引起的“模糊”吸收线。它的年龄大约9,400万[7]，并且有185公里/秒的投影自转速度[9]，估计它的质量是太阳质量的3.4倍[8]，来自光球的有效温度为13,781K [9]，使它辐射的光度是太阳光度的153倍[8]。 它有一颗紧密的伴星，是 X射线发射的来源。这颗恒星的质量很可能至少是太阳的1.05倍[7]。第三颗星是天兔座AM，是一颗天龙座BY型变星[11]，视星等9.92等 [3]，光谱类行为G8Ve[12]，角距离12.7"[13]。
参考资料 编辑
- ^ Huélamo, N.; Fernández, M.; Neuhäuser, R.; Wolk, S. J. Rotation periods of Post-T Tauri stars in Lindroos systems (PDF). Astronomy and Astrophysics. December 2004, 428 (3): 953–967 [29 June 2022]. Bibcode:2004A&A...428..953H. S2CID 10656237. arXiv:astro-ph/0408226
. doi:10.1051/0004-6361:20034442. （原始内容存档 (PDF)于2023-10-28）.
- ^ 2.0 2.1 2.2 2.3 2.4 2.5 van Leeuwen, F., Validation of the new Hipparcos reduction, Astronomy and Astrophysics, 2007, 474 (2): 653–664, Bibcode:2007A&A...474..653V, S2CID 18759600, arXiv:0708.1752 , doi:10.1051/0004-6361:20078357.
- ^ 3.0 3.1 3.2 3.3 3.4 Ducati, J. R., VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system, CDS/ADC Collection of Electronic Catalogues, 2002, 2237: 0, Bibcode:2002yCat.2237....0D.
- ^ 4.0 4.1 Garrison, R. F.; et al, The late B-type stars: refined MK classification, confrontation with Stromgren photometry, and the effects of rotation, The Astronomical Journal, 1994, 107 (4): 1556–1564, Bibcode:1994AJ....107.1556G, doi:10.1086/116967.
- ^ 5.0 5.1 Eggleton, P. P.; Tokovinin, A. A., A catalogue of multiplicity among bright stellar systems, Monthly Notices of the Royal Astronomical Society, September 2008, 389 (2): 869–879, Bibcode:2008MNRAS.389..869E, S2CID 14878976, arXiv:0806.2878 , doi:10.1111/j.1365-2966.2008.13596.x.
- ^ Kharchenko, N. V.; et al, Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ˜55000 stars and mean radial velocities of 516 Galactic open clusters and associations, Astronomische Nachrichten, 2007, 328 (9): 889, Bibcode:2007AN....328..889K, S2CID 119323941, arXiv:0705.0878 , doi:10.1002/asna.200710776.
- ^ 7.0 7.1 7.2 7.3 Hubrig, S.; et al, Search for low-mass PMS companions around X-ray selected late B stars, Astronomy and Astrophysics, June 2001, 372: 152–164, Bibcode:2001A&A...372..152H, S2CID 17507782, arXiv:astro-ph/0103201 , doi:10.1051/0004-6361:20010452.
- ^ 8.0 8.1 8.2 8.3 Zorec, J.; Royer, F., Rotational velocities of A-type stars. IV. Evolution of rotational velocities, Astronomy & Astrophysics, January 2012, 537: A120, Bibcode:2012A&A...537A.120Z, S2CID 55586789, arXiv:1201.2052 , doi:10.1051/0004-6361/201117691.
- ^ 9.0 9.1 9.2 9.3 9.4 David, Trevor J.; Hillenbrand, Lynne A., The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets, The Astrophysical Journal, 2015, 804 (2): 146, Bibcode:2015ApJ...804..146D, S2CID 33401607, arXiv:1501.03154 , doi:10.1088/0004-637X/804/2/146.
- ^ [ iot Lep] 请检查
|url=值 (帮助). SIMBAD. 斯特拉斯堡天文资料中心. [2017-08-18]. - ^ Kazarovets, E. V.; et al, The 79th name-list of variable stars, Information Bulletin on Variable Stars, 2008, 5863 (1): 1, Bibcode:2008IBVS.5863....1K.
- ^ Gahm, G. F.; et al, A study of visual double stars with early type primaries. I - Spectroscopic results, Astronomy and Astrophysics Supplement Series, 1983, 51: 143–159, Bibcode:1983A&AS...51..143G.
- ^ Dommanget, J.; et al, Catalog of Components of Double & Multiple stars, Observations et Travaux, 2002, 54 (5), Bibcode:2002yCat.1274....0D. Vizier result （页面存档备份，存于互联网档案馆）
