巨蛇座R
| 观测资料 历元 J2000 | |
|---|---|
| 星座 | 巨蛇座 |
| 星官 | |
| 赤经 | 15h 50m 41.73245s[2] |
| 赤纬 | +15° 08′ 01.0810″[2] |
| 视星等（V） | 9.70[3] |
| 特性 | |
| 光谱分类 | M5-8e[4] |
| B−V 色指数 | 1.500±0.510[3] |
| 变星类型 | 米拉[5] |
| 天体测定 | |
| 径向速度 (Rv) | 23.8±0.8[6] km/s |
| 自行 (μ) | 赤经：+2.387[2] mas/yr 赤纬：−36.699[2] mas/yr |
| 视差 (π) | 3.5110 ± 0.2966[2] mas |
| 距离 | 930 ± 80 ly (280 ± 20 pc) |
| 详细资料 | |
| 半径 | ~380[7] R☉ |
| 亮度 | 1,704.70[8] L☉ |
| 温度 | 2,780±80[9] K |
| 其他命名 | |
| 参考资料库 | |
| SIMBAD | 资料 |
巨蛇座R是在赤道星座巨蛇座的一颗蒭藁型变星。它的视星等在5.16和14.4等之间变化，光谱类型在M5e至M8e变动，周期为356.41日[5][11]。卡尔·路德维希·哈丁在1826年发现这颗恒星是颗变星[12]。
参考资料
[编辑]- ^ Download Data. aavso.org. AAVSO. [1 October 2021]. （原始内容存档于2023-03-15）.
- ^ 2.0 2.1 2.2 2.3 2.4 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.
- ^ 3.0 3.1 Anderson, E.; Francis, Ch., XHIP: An extended hipparcos compilation, Astronomy Letters, 2012, 38 (5): 331, Bibcode:2012AstL...38..331A, S2CID 119257644, arXiv:1108.4971 , doi:10.1134/S1063773712050015.
- ^ Keenan, Philip C.; et al, Revised Catalog of Spectra of Mira Variables of Types ME and Se, Astrophysical Journal Supplement, 1974, 28: 271, Bibcode:1974ApJS...28..271K, doi:10.1086/190318 .
- ^ 5.0 5.1 Samus', N. N; Kazarovets, E. V; Durlevich, O. V; Kireeva, N. N; Pastukhova, E. N, General catalogue of variable stars: Version GCVS 5.1, Astronomy Reports, 2017, 61 (1): 80, Bibcode:2017ARep...61...80S, S2CID 125853869, doi:10.1134/S1063772917010085.
- ^ Gontcharov, G. A., Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system, Astronomy Letters, November 2006, 32 (11): 759–771, Bibcode:2006AstL...32..759G, S2CID 119231169, arXiv:1606.08053 , doi:10.1134/S1063773706110065.
- ^ Pasinetti Fracassini, L. E.; et al, Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS), Astronomy and Astrophysics Third, February 2001, 367: 521–524, Bibcode:2001A&A...367..521P, S2CID 425754, arXiv:astro-ph/0012289 , doi:10.1051/0004-6361:20000451.
- ^ McDonald, I.; et al, Fundamental parameters and infrared excesses of Hipparcos stars, Monthly Notices of the Royal Astronomical Society, 2012, 427 (1): 343–357, Bibcode:2012MNRAS.427..343M, S2CID 118665352, arXiv:1208.2037 , doi:10.1111/j.1365-2966.2012.21873.x.
- ^ Hofmann, K. -H.; et al, Observations of Mira stars with the IOTA/FLUOR interferometer and comparison with Mira star models, New Astronomy, January 2002, 7 (1): 9–20, Bibcode:2002NewA....7....9H, S2CID 14854720, arXiv:astro-ph/0004013 , doi:10.1016/S1384-1076(01)00085-9.
- ^ R Ser. SIMBAD. 斯特拉斯堡天文资料中心.
- ^ Watson, Christopher. R Serpentis. AAVSO Website. American Association of Variable Star Observers. 4 January 2010 [22 May 2014]. （原始内容存档于2021-05-16）.
- ^ Zsoldos, E. Three Early Variable Star Catalogues. Journal for the History of Astronomy. 1994, 25 (2): 92–98 [2023-10-27]. Bibcode:1994JHA....25...92Z. S2CID 117099222. doi:10.1177/002182869402500202. （原始内容存档于2023-10-28）.
