HD 38529
出典: フリー百科事典『ウィキペディア（Wikipedia）』 (2024/01/04 20:27 UTC 版)
HD 38529は、オリオン座の方角におよそ138光年離れた位置にある連星系である[3][10]。主星の周りには、太陽系外惑星が1つ、褐色矮星が1つみつかっており、それらを取り巻く残骸円盤も存在するとみられる[1][11][12]。
注釈
![{\displaystyle \log g[{\mbox{cgs}}]=3.77}](http://weblio.hs.llnwd.net/e7/img/dict/wkpja/https://wikimedia.org/api/rest_v1/media/math/render/svg/1572df4befabf0a603898f4444148a6a1694acb6)
出典
- ^ a b c d e f g Fischer, Debra A.; et al. (2001-04), “Planetary Companions to HD 12661, HD 92788, and HD 38529 and Variations in Keplerian Residuals of Extrasolar Planets”, Astrophysical Journal 551 (2): 1107-1118, Bibcode: 2001ApJ...551.1107F, doi:10.1086/320224
- ^ a b Zacharias, N.; et al. (2013-02), “The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)”, Astronomical Journal 145 (2): 44, Bibcode: 2013AJ....145...44Z, doi:10.1088/0004-6256/145/2/44
- ^ a b c d e f g h “HD 38529 -- High proper-motion Star”. SIMBAD. CDS. 2021年3月16日閲覧。
- ^ a b c d e f g Luhn, Jacob K.; et al. (2019-04), “Retired A Stars and Their Companions. VIII. 15 New Planetary Signals around Subgiants and Transit Parameters for California Planet Search Planets with Subgiant Hosts”, Astronomical Journal 157 (4): 149, Bibcode: 2019AJ....157..149L, doi:10.3847/1538-3881/aaf5d0
- ^ a b Terrien, Ryan C.; et al. (2015-09), “A Near-Infrared Spectroscopic Survey of 886 Nearby M Dwarfs”, Astrophysical Journal Supplement Series 220 (1): 16, Bibcode: 2015ApJS..220...16T, doi:10.1088/0067-0049/220/1/16
- ^ a b c d e f Xuan, Jerry W.; et al. (2020-10), “Mutual inclinations between giant planets and their debris discs in HD 113337 and HD 38529”, Monthly Notices of the Royal Astronomical Society 499 (4): 5059-5074, Bibcode: 2020MNRAS.499.5059X, doi:10.1093/mnras/staa3155
- ^ a b c d e f Henry, Gregory W.; et al. (2013-05), “Host Star Properties and Transit Exclusion for the HD 38529 Planetary System”, Astrophysical Journal 768 (2): 155, Bibcode: 2013ApJ...768..155H, doi:10.1088/0004-637X/768/2/155
- ^ a b Alonso-Floriano, F. J.; et al. (2015-05), “CARMENES input catalogue of M dwarfs. I. Low-resolution spectroscopy with CAFOS”, Astronomy & Astrophysics 577: A128, Bibcode: 2015A&A...577A.128A, doi:10.1051/0004-6361/201525803
- ^ a b Veyette, Mark J.; et al. (2017-12), “A Physically Motivated and Empirically Calibrated Method to Measure the Effective Temperature, Metallicity, and Ti Abundance of M Dwarfs”, Astrophysical Journal 851 (1): 26, Bibcode: 2017ApJ...851...26V, doi:10.3847/1538-4357/aa96aa
- ^ a b Raghavan, Deepak; et al. (2006-07), “Two Suns in The Sky: Stellar Multiplicity in Exoplanet Systems”, Astrophysical Journal 646 (1): 523-542, Bibcode: 2006ApJ...646..523R, doi:10.1086/504823
- ^ a b Benedict, G. Fritz; et al. (2010-05), “The Mass of HD 38529c from Hubble Space Telescope Astrometry and High-precision Radial Velocities”, Astronomical Journal 139 (5): 1844-1856, Bibcode: 2010AJ....139.1844B, doi:10.1088/0004-6256/139/5/1844
- ^ a b Moro-Martín, Amaya; et al. (2007-10), “The Dust, Planetesimals, and Planets of HD 38529”, Astrophysical Journal 668 (2): 1165-1173, Bibcode: 2007ApJ...668.1165M, doi:10.1086/521093
- ^ “HD 38529B -- High proper-motion Star”. SIMBAD. CDS. 2021年3月16日閲覧。
- ^ Fischer, Debra A.; et al. (2003-04), “A Planetary Companion to HD 40979 and Additional Planets Orbiting HD 12661 and HD 38529”, Astrophysical Journal 586 (2): 1394-1408, Bibcode: 2003ApJ...586.1394F, doi:10.1086/367889
[続きの解説]
「HD 38529」の続きの解説一覧
- 1 HD 38529とは
- 2 HD 38529の概要
- 3 星系
- 4 関連項目
「HD 38529」の例文・使い方・用例・文例
- HD 38529のページへのリンク
