天鹅座X
| 观测资料 历元 J2000 | |
|---|---|
| 星座 | 天鹅座 |
| 星官 | |
| 赤经 | 20h 43m 24.192s[2] |
| 赤纬 | 35° 35′ 16.08″[2] |
| 视星等（V） | 5.85 to 6.91[3] |
| 特性 | |
| 光谱分类 | F7 Ib to G8 Ib[4] |
| 变星类型 | 仙王座δ[3] |
| 天体测定 | |
| 径向速度 (Rv) | 8.1+0.2 −[5] km/s |
| 自行 (μ) | 赤经：−6.673 mas/yr 赤纬：−5.108 mas/yr |
| 视差 (π) | 0.8842 ± 0.0199[2] mas |
| 距离 | 3,690 ± 80 ly (1,130 ± 30 pc) |
| 绝对星等 (MV) | −4.53[6] |
| 详细资料 | |
| 质量 | 7.9–8.9[7] M☉ |
| 半径 | 95.9+1.6 −[8] R☉ |
| 表面重力 (log g) | 1.601[9] |
| 亮度 | 5,202[10] L☉ |
| 温度 | 5,315+80 −[8] K |
| 金属量 [Fe/H] | 0.10+0.08 −[8] dex |
| 自转速度 (v sin i) | 8[7] km/s |
| 年龄 | 31[6] Myr |
| 其他命名 | |
| 参考资料库 | |
| SIMBAD | 资料 |
天鹅座X是在星座天鹅座北部的一颗变星，英文缩写为X Cyg。这是一颗仙王座δ型变星，其视星等的亮度范围从5.85到6.91的，周期为16.386332天[3]。在最亮的时候，这颗恒星肉眼隐约可见。根据视差的量测，到这颗恒星的距离约为628光年[2]。它正以8.1km/s的径向速度远离我们[5]。这颗恒星很可能是疏散星团鲁普雷希特173的成员[12]。
这颗恒星的变星光度是由小赛斯·卡罗·钱德勒于1886年发现的[13]。在1907年，埃德温·布兰特·弗罗斯特表明，天鹅座X是一颗F型恒星，具有不同的径向速度，其行为类似于仙王座δ变星[14]。米歇尔·路易泽在1912年发现，这种变化的周期为16.38543天[15]。在1919年，弗兰克·克雷格·乔丹确定恒星的色指数在每个周期中都会发生变化，随著恒星变暗而变红[16]。它被确定为满足简单周光关系的基准恒星类别经典造父变星的成员[17]。
在1954年，罗伯特·克拉夫特在峰值亮度下发现其恒星分类为F7-Ib[18]，与F型超巨星的光谱相匹配。这颗恒星的光谱类型在脉动周期中变化，在最小亮度下低至G8 Ib[4]。在1956年，克拉夫特发现某些谱线加倍，他解释说这是由于之前的脉动周期中，物质壳下落与光球碰撞的结果[19]。与大多数造父变星在每个周期经历一次冲击不同，天鹅座X被发现经历了一次双重冲击[20]。
现时还没有发现轨道周期在十年或更短的伴星[21]。这颗恒星显示出卷云，并初步证明了红外的长期发射[22]。
参考资料
- ^ MAST: Barbara A. Mikulski Archive for Space Telescopes, Space Telescope Science Institute, [30 December 2022].
- ^ 2.0 2.1 2.2 2.3 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. - ^ 3.0 3.1 3.2 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.
- ^ 4.0 4.1 Kovtyukh, V. V.; et al, Phase-dependent Variation of the Fundamental Parameters of Cepheids. II. Periods Longer than 10 Days, The Astronomical Journal, January 2005, 129 (1): 433–453, Bibcode:2005AJ....129..433K, S2CID 120666782, doi:10.1086/426339 .
- ^ 5.0 5.1 Gontcharov, G. A., Pulkovo Compilation of Radial Velocities for 35495 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.
- ^ 6.0 6.1 Acharova, I. A.; et al, Galactic restrictions on iron production by various types of supernovae, Monthly Notices of the Royal Astronomical Society, 2012, 420 (2): 1590, Bibcode:2012MNRAS.420.1590A, S2CID 118404944, arXiv:1111.2152 , doi:10.1111/j.1365-2966.2011.20161.x.
- ^ 7.0 7.1 Breitfellner, M. G.; Gillet, D., Atmospheric motions in classical cepheid stars. III. A very large amplitude star : X Cygni, Astronomy and Astrophysics, October 1993, 277: 553, Bibcode:1993A&A...277..553B.
- ^ 8.0 8.1 8.2 Trahin, B.; et al, Inspecting the Cepheid parallax of pulsation using Gaia EDR3 parallaxes. Projection factor and period-luminosity and period-radius relations, Astronomy & Astrophysics, December 2021, 656, Bibcode:2021A&A...656A.102T, S2CID 244173657, arXiv:2111.09125 , doi:10.1051/0004-6361/202141680, A102.
- ^ Sprague, Dani; et al, APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars, The Astronomical Journal, March 8, 2022, 163 (4): 152, Bibcode:2022AJ....163..152S, ISSN 0004-6256, arXiv:2201.03661 , doi:10.3847/1538-3881/ac4de7 , eISSN 1538-3881.
- ^ Groenewegen, M. A. T., The flux-weighted gravity-luminosity relation of Galactic classical Cepheids, Astronomy and Astrophysics, 2020, 640: A113, Bibcode:2020A&A...640A.113G, S2CID 220364506, arXiv:2007.02148 , doi:10.1051/0004-6361/202038292.
- ^ [ X Cyg] 请检查
|url=值 (帮助). SIMBAD. 斯特拉斯堡天文资料中心. - ^ Anderson, Richard I.; et al, Cepheids in open clusters: an 8D all-sky census, Monthly Notices of the Royal Astronomical Society, September 2013, 434 (3): 2238–2261, Bibcode:2013MNRAS.434.2238A, arXiv:1212.5119 , doi:10.1093/mnras/stt1160.
- ^ Chandler, S. C., On a new short-period variable in Cygnus, Astronomical Journal, December 1886, 7 (148): 32, Bibcode:1886AJ......7...32C, doi:10.1086/100855.
- ^ Frost, E. B., Nine stars having variable radial velocities, Astrophysical Journal, 1907, 25: 59–65, Bibcode:1907ApJ....25R..59F, doi:10.1086/141465.
- ^ Luizet, Michel, Nouveaux éléments et courbes de lumière des étoiles X Cygni et RU Camelopardalis, Astronomische Nachrichten, November 1912, 193 (6): 83, Bibcode:1912AN....193...83L, doi:10.1002/asna.19121930603 （法语）.
- ^ Jordan, F. C., The color changes of certain variable stars of short period, Astrophysical Journal, October 1919, 50: 174–205, Bibcode:1919ApJ....50..174J, doi:10.1086/142495, hdl:2027/mdp.39015086631564 .
- ^ Eggen, Olin J., Photoelectric Studies. V. Magnitudes and Colors of Classical Cepheid Variable Stars, Astrophysical Journal, March 1951, 113: 367, Bibcode:1951ApJ...113..367E, doi:10.1086/145405 .
- ^ Kraft, Robert P., Changes in the Spectrum of X Cygni, Publications of the Astronomical Society of the Pacific, June 1954, 66 (390): 136, Bibcode:1954PASP...66..136K, S2CID 123620740, doi:10.1086/126679.
- ^ Kraft, Robert P., Double Lines in the Spectrum of the Classical Cepheid X Cygni, Publications of the Astronomical Society of the Pacific, April 1956, 68 (401): 137, Bibcode:1956PASP...68..137K, S2CID 122849355, doi:10.1086/126897 .
- ^ Gillet, D., Atmospheric dynamics in long-period Cepheids. Hα profile variations, Astronomy & Astrophysics, August 2014, 568, Bibcode:2014A&A...568A..72G, doi:10.1051/0004-6361/201423486 , A72.
- ^ Hintz, Eric G.; et al, An Examination of Pulsational Changes in the Classical Cepheid X Cygni, The Astronomical Journal, October 2021, 162 (4): 149, Bibcode:2021AJ....162..149H, S2CID 237553133, doi:10.3847/1538-3881/ac167f , 149.
- ^ Barmby, P.; et al, Galactic Cepheids with Spitzer. II. Search for Extended Infrared Emission, The Astronomical Journal, February 2011, 141 (2): 42, Bibcode:2011AJ....141...42B, S2CID 118581168, arXiv:1011.3386 , doi:10.1088/0004-6256/141/2/42, 42.
进阶读物
- Wallerstein, G.; et al, The Behavior of the Paschen and Calcium Triplet Lines in Cepheid Variables II: The 16-day Variable X Cygni, Publications of the Astronomical Society of the Pacific, September 2019, 131 (1003): 094203, Bibcode:2019PASP..131i4203W, S2CID 201259492, doi:10.1088/1538-3873/ab1ec2 .
- Meyer, Ralf, X Cyg: observations from 1886 until today, Open European Journal on Variable Stars, December 2005, 13: 1, Bibcode:2005OEJV...13....1M.
- Turner, David G., A Search for Stars Physically Associated with the 16 Day Cepheid X Cygni. II. Clusters in the Field, The Astronomical Journal, July 1998, 116 (1): 274–283, Bibcode:1998AJ....116..274T, S2CID 123331380, doi:10.1086/300438 .
- Wallerstein, G.; et al, A search for evidence of the neon-sodium cycle in the Cepheid X Cygni, Publications of the Astronomical Society of the Pacific, August 1984, 96: 613–617, Bibcode:1984PASP...96..613W, S2CID 120641485, doi:10.1086/131392.
- Evans, N. R., X Cygni: duplicity, period stability and atmospheric velocity structure, Astrophysical Journal, June 1984, 281: 760–765, Bibcode:1984ApJ...281..760E, doi:10.1086/162154 .
- Wallerstein, G., The behavior of H alpha in the 16-day cepheid X Cygni, Publications of the Astronomical Society of the Pacific, July 1983, 95: 422–426, Bibcode:1983PASP...95..422W, S2CID 122893194, doi:10.1086/131187 .
- Turner, D. G., A search for stars physically associated with the 16-day Cepheid X Cygni. I. Luminous Stars in the field, Astronomical Journal, May 1983, 88: 650–654, Bibcode:1983AJ.....88..650T, doi:10.1086/113353.
- Benz, W.; Mayor, M., Turbulence variations for the three cepheids SV Vul, X CYG and del Cep, Astronomy and Astrophysics, July 1982, 111: 224–228, Bibcode:1982A&A...111..224B.
- Davis, C. G.; et al, On the mass of the cepheid X Cyg, Astrophysical Journal, June 1981, 246: 914–918, Bibcode:1981ApJ...246..914D, doi:10.1086/158984.
- Abt, H. A., Radial velocities of the cepheid X Cygni, Publications of the Astronomical Society of the Pacific, June 1978, 90: 309–311, Bibcode:1978PASP...90..309A, S2CID 120199788, doi:10.1086/130332 .
- Masani, A.; et al, The Masses of BM Cas, X Cyg, RT Aur, RR Lyr, Information Bulletin on Variable Stars, February 1968, 258: 1, Bibcode:1968IBVS..258....1M.
- Masani, A.; et al, Determination of the Mass and the Model of the Variables: RT Aurigae, Eta Aquilae, X Cygni, Mira Ceti and BM Cassiopeiae of Pop.I, and RR Lyrae and Two Typical Variables of Pop. II, Information Bulletin on Variable Stars, October 1966, 162: 1, Bibcode:1966IBVS..162....1M.
- Duncan, J. C., The spectroscopic orbit of the cepheid variable X Cygni, Astrophysical Journal, January 1921, 53: 95–98, Bibcode:1921ApJ....53...95D, doi:10.1086/142585.