白羊座UX
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觀測資料 曆元 J2000
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星座
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白羊座
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星官
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赤經
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03h 26m 35.37568s[2]
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赤緯
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+28° 42′ 54.2264″[2]
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視星等(V)
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6.35 - 6.71[3]
| 特性 |
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光谱分类 | G5IV[4] | U−B 色指数 | 0.43[5] | B−V 色指数 | 0.90[5] | 变星类型 | RS CVn[6] |
天体测定 |
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徑向速度 (Rv) | +26.53[7] km/s | 自行 (μ) | 赤经:+46.794[2] mas/yr 赤纬:−102.876[2] mas/yr | 视差 (π) | 19.7836 ± 0.1264[2] mas | 距离 | 165 ± 1 ly (50.5 ± 0.3 pc) | 绝对星等 (MV) | 2.91[8] | |
軌道[9] | 主星 | Aa | 伴星 | Ab | 繞行週期 (P) | 7005556233523200000♠6.437888±0.000007 d | 半長軸 (a) | 6991848423941941689♠1.750±0.01 mas | 偏心率 (e) | 0 (fixed) | 倾斜角 (i) | 7002125000000000000♠125.0±0.5° | 升交点黃經 (Ω) | 7002113400000000000♠113.4±0.4° | 近心点 曆元 (T) | 2456238.134 ± 0.002 HJD | 近心點幅角 (ω) (secondary) | 90(確定的)° |
軌道[10] | 主星 | A | 伴星 | B | 繞行週期 (P) | 111.02 yr | 半長軸 (a) | 6994314159265358980♠648.0±0.8 mas | 偏心率 (e) | 6999770000000000000♠0.77±0.01 | 倾斜角 (i) | 7001933000000000000♠93.3±0.6° | 升交点黃經 (Ω) | 7001589000000000000♠58.9±0.5° | 近心点 曆元 (T) | 7006245166490000000♠2451664.9±34.3 HJD | 近心點幅角 (ω) (secondary) | 7002274899999999999♠274.9±0.8° |
詳細資料 [9]
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白羊座UX Aa
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質量 | 7000130000000000000♠1.30±0.06 M☉ | 半徑 | 7000559999999999999♠5.6±0.1 R☉ | 表面重力 (log g) | 7000306000000000000♠3.06±0.04 | 亮度 | 7000930000000000000♠9.3±0.7 L☉ | 溫度 | 7003456000000000000♠4,560±100 K | 自轉 | 6.44 d[4] |
白羊座UX Ab
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質量 | 7000113999999999999♠1.14±0.06 M☉ | 半徑 | 7000160000000000000♠1.6±0.2 R☉ | 表面重力 (log g) | 7000409000000000000♠4.09±0.16 | 亮度 | 7000234000000000000♠2.34±0.28 L☉ | 溫度 | 7003567000000000000♠5,670±100 K |
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白羊座UX B
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質量 | 0.75 M☉ | 半徑 | 6999800000000000000♠0.8±0.1 R☉ | 表面重力 (log g) | 7000451000000000000♠4.51±0.13 | 亮度 | 6999380000000000000♠0.38±0.08 L☉ | 溫度 | 7003493000000000000♠4,930±100 K |
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其他命名
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| 參考資料庫 |
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SIMBAD | 资料 | ARICNS | 资料 |
白羊座UX是在北天的黃道星座白羊座的一個三合星系統。基於來自蓋亞衛星的視差測量,它距離太陽系大約165光年。主星,白羊座UX Aa,是一顆RS CVn型變星。這顆恆星的光度變化被認為是由於冷星斑和溫暖的耀斑組合,與恆星大氣層的基態溫度相對照。這種變化似乎是週期性,週期為8-9年[6]。這顆恆星的亮度從視星等6.35到6.71不等,這意味著在理想的黑暗天空條件下,肉眼可能會間歇性地看到它[3]。
一顆更遠的伴星,成員C,有著共同自行,並且處於相同的距離上[11]。它是另一顆冷矮星,估計光譜等級為K2。任何一種估計的軌道都超過10萬年[12]。
參考資料
- ^ Ulvås, V. Aarum; Henry, G. W. BV photometry of UX Ari in the period 1987–2002. Astronomy & Astrophysics. May 2003, 402 (3): 1033–1041. Bibcode:2003A&A...402.1033A. doi:10.1051/0004-6361:20030304 .
- ^ 2.0 2.1 2.2 2.3 2.4 Vallenari, A.; et al. Gaia Data Release 3. Summary of the content and survey properties. Astronomy & Astrophysics. 2022. arXiv:2208.00211 . doi:10.1051/0004-6361/202243940 . Gaia DR3 record for this source at VizieR.
- ^ 3.0 3.1 UX Ari. The International Variable Star Index. AAVSO. [28 October 2021]. (原始内容存档于2021-10-29).
- ^ 4.0 4.1 Strassmeier, Klaus G. Starspots. The Astronomy and Astrophysics Review. September 2009, 17 (3): 251–308. Bibcode:2009A&ARv..17..251S. doi:10.1007/s00159-009-0020-6 .
- ^ 5.0 5.1 Guetter, H. H.; Hewitt, A. V. Photoelectric UBV photometry for 317 PZT and VZT stars. Publications of the Astronomical Society of the Pacific. June 1984, 96: 441–443. Bibcode:1984PASP...96..441G. doi:10.1086/131362 .
- ^ 6.0 6.1 Alekseev, I. Yu. Three-Component Model of Spottedness in the Classical RS CVn System UX Ari. Astrophysics. September 2014, 57 (3): 344–351. Bibcode:2014Ap.....57..344A. S2CID 119963417. doi:10.1007/s10511-014-9339-4.
- ^ Karataș, Yüksel; Bilir, Selçuk; Eker, Zeki; Demircan, Osman; Liebert, James; Hawley, Suzanne L.; Fraser, Oliver J.; Covey, Kevin R.; Lowrance, Patrick; Kirkpatrick, J. Davy; Burgasser, Adam J. Kinematics of chromospherically active binaries and evidence of an orbital period decrease in binary evolution. Monthly Notices of the Royal Astronomical Society. 2004, 349 (3): 1069–1092. Bibcode:2004MNRAS.349.1069K. S2CID 15290475. arXiv:astro-ph/0404219 . doi:10.1111/j.1365-2966.2004.07588.x.
- ^ Anderson, E.; Francis, Ch. XHIP: An extended hipparcos compilation. Astronomy Letters. May 2012, 38 (5): 331–346. Bibcode:2012AstL...38..331A. ISSN 1063-7737. S2CID 119257644. arXiv:1108.4971 . doi:10.1134/S1063773712050015. eISSN 1562-6873.
- ^ 9.0 9.1 Hummel, C. A.; et al. Orbital Elements and Stellar Parameters of the Active Binary UX Arietis. The Astrophysical Journal. August 2017, 844 (2): 12. Bibcode:2017ApJ...844..115H. S2CID 43383613. doi:10.3847/1538-4357/aa7b87. hdl:10871/32318 . 115.
- ^ Peterson, W. M.; Mutel, R. L.; Lestrade, J. -F.; Güdel, M.; Goss, W. M. Radio Astrometry of the Triple Systems Algol and UX Arietis. The Astrophysical Journal. 2011, 737 (2): 104. Bibcode:2011ApJ...737..104P. S2CID 119229905. arXiv:1104.5005 . doi:10.1088/0004-637X/737/2/104.
- ^ Vallenari, A.; et al. Gaia Data Release 3. Summary of the content and survey properties. Astronomy & Astrophysics. 2022. arXiv:2208.00211 . doi:10.1051/0004-6361/202243940 . Gaia DR3 record for this source at VizieR.
- ^ Tokovinin, Andrei. The Updated Multiple Star Catalog. The Astrophysical Journal Supplement Series. 2018-03-01, 235 (1): 6. Bibcode:2018ApJS..235....6T. ISSN 0067-0049. S2CID 119047709. arXiv:1712.04750 . doi:10.3847/1538-4365/aaa1a5.
進階讀物
外部連結
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