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CARMENES science preparation: characterisation of M dwarfs with low-resolution spectroscopy and search for low-mass wide companions to young stars

机译：卡门尼斯科学准备：使用低分辨率光谱表征M矮星，并寻找年轻恒星的低质量宽伴星

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Alonso Floriano Francisco Javier;
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年度 2015
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1. PLANETS AROUND LOW-MASS STARS (PALMS). II. A LOW-MASS COMPANION TO THE YOUNG M?DWARF GJ?3629 SEPARATED BY 0.″2* [J] . Brendan P. Bowler, Michael C. Liu, Evgenya L. Shkolnik, The Astrophysical journal . 2012,第1期

机译：低质量恒星（PALMS）周围的行星。二。与年轻M？DWARF GJ？3629的低质量同伴，以0.″ 2 *分隔
2. PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT*, ** [J] . Brendan P. Bowler, Michael C. Liu, Evgenya L. Shkolnik, The Astrophysical journal . 2013,第1期

机译：低质量恒星周围的行星。三，氘燃烧极限*的年轻尘埃杜瓦夫同伴**
3. PLANETS AROUND LOW-MASS STARS (PALMS). I. A SUBSTELLAR COMPANION TO THE YOUNG M DWARF 1RXS J235133.3+312720* [J] . Brendan P. Bowler, Michael C. Liu, Evgenya L. Shkolnik, The Astrophysical journal . 2012,第2期

机译：低质量恒星（PALMS）周围的行星。 I.与年轻M DWARF 1RXS J235133.3 + 312720 *形成的同伴
4. Circumstellar disk fragmentation and the origin of massive planetary companions, brown dwarfs, and very low-mass stars [C] . M. B. N. Kouwenhoven, Yun Li, D. Stamatellos, Symposium of the International Astronomical Union;International Astronomical Union., Symposium . 2019

机译：Scrayellar盘碎片和大规模行星伴侣的起源，棕色矮人和非常低质量的恒星
5. Characterizing Cool Brown Dwarfs and Low-Mass Companions with Low-Resolution Near-Infrared Spectra [D] . Godfrey, Paige A. 2017

机译：用低分辨率近红外光谱表征酷棕色矮人和低质量伴侣
6. DISCOVERY OF TWO VERY WIDE BINARIES WITH ULTRACOOL COMPANIONS AND A NEW BROWN DWARF AT THE L/T TRANSITION [O] . Koraljka Mužić, Jacqueline Radigan, Ray Jayawardhana, -1

机译：TWO的发现非常宽的二进制码采用超级酷的同伴和一种新的褐矮在L / T TRaNsITION
7. Planets Around Low-Mass Stars (PALMS). II. A Low-Mass Companion to the Young M Dwarf GJ 3629 Separated By 0.2" [O] . Bowler, Brendan P., Liu, Michael C., Shkolnik, Evgenya L., 2012

机译：低质量恒星周围的行星（paLms）。 II。一个低质量的伴侣 Young m矮人GJ 3629分开0.2“

CARMENES science preparation: characterisation of M dwarfs with low-resolution spectroscopy and search for low-mass wide companions to young stars

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