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  • 标题:Spectroscopic Orbits of 11 Nearby, Mid-to-late M-dwarf Binaries
  • 本地全文:下载
  • 作者:Jennifer G.Winters ; Jonathan M.Irwin ; David Charbonneau
  • 期刊名称:The Astronomical journal
  • 印刷版ISSN:0004-6256
  • 电子版ISSN:1538-3881
  • 出版年度:2020
  • 卷号:159
  • 期号:6
  • 页码:4054-4067
  • DOI:10.3847/1538-3881/ab8d31
  • 语种:English
  • 出版社:American Institute of Physics
  • 摘要:We present the spectroscopic orbits of 11 nearby, mid-to-late M dwarf binary systems in a variety of configurations: 2 single-lined binaries (SB1s), 7 double-lined binaries (SB2s), 1 double-lined triple (ST2), and 1 triple-lined triple (ST3).Eight of these orbits are the first published for these systems, while five are newly identified multiples.We obtained multi-epoch, high-resolution spectra with the TRES instrument on the 1.5 m Tillinghast Reflector at the Fred Lawrence Whipple Observatory located on Mt.Hopkins in AZ.Using the TiO molecular bands at 7065−7165 Å, we calculated radial velocities for these systems, from which we derived their orbits.We find LHS 1817 to have in a 7 hr period a companion that is likely a white dwarf, due to the ellipsoidal modulation we see in our MEarth-North light-curve data.We find G 123-45 and LTT 11586 to host companions with minimum masses of 41 MJup and 44 MJup with orbital periods of 35 and 15 days, respectively.We find 2MA 0930+0227 to have a rapidly rotating stellar companion in a 917 day orbital period.GJ 268, GJ 1029, LP 734-34, GJ 1182, G 258-17, and LTT 7077are SB2s with stellar companions with orbital periods of 10, 96, 34, 154, 5, and 84 days; LP 655-43 is an ST3 with one companion in an 18 day orbital period and an outer component in a longer undetermined period.In addition, we present radial velocities for both components of L 870-44AB and for the outer components of LTT 11586 and LP 655-43.
  • 关键词:Spectroscopic binary stars;Solar neighborhood;M dwarf stars;White dwarf stars;Orbital elements;Substellar companion stars
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