巨蛇座R是在赤道星座巨蛇座的一顆蒭藁型變星。它的視星等在5.16和14.4等之間變化,光譜類型在M5e至M8e變動,週期為356.41日[5][11]卡爾·路德維希·哈丁在1826年發現這顆恆星是顆變星[12]

巨蛇座R

來自AAVSO數據的巨蛇座R的可見光光變曲線[1]
觀測資料
曆元 J2000
星座 巨蛇座
星官
赤經 15h 50m 41.73245s[2]
赤緯 +15° 08′ 01.0810″[2]
視星等(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
徑向速度 (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)
詳細資料
半徑~380[7] R
亮度1,704.70[8] L
溫度2,780±80[9] K
其他命名
R Ser、​BD+15° 2918、​HD 141850、​HIP 77615、​HR 5894、​SAO 101771[10]
參考資料庫
SIMBAD资料

參考資料

  1. ^ Download Data. aavso.org. AAVSO. [1 October 2021]. (原始内容存档于2023-03-15). 
  2. ^ 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. ^ 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. 
  4. ^ 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. ^ 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. 
  6. ^ 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. 
  7. ^ 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. 
  8. ^ 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. 
  9. ^ 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. 
  10. ^ R Ser. SIMBAD. 斯特拉斯堡天文資料中心. 
  11. ^ 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). 
  12. ^ 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).