M dwarf stars in the light of (future) exoplanet searches

被引：5

作者：

Rojas-Ayala, B. ^{[1
]}

Hilton, E. J. ^{[2
,3
]}

Mann, A. W. ^{[2
]}

Lepine, S. ^{[1
]}

Gaidos, E. ^{[3
]}

Bonfils, X. ^{[4
]}

Helling, Ch ^{[5
]}

Henry, T. J. ^{[6
]}

Rogers, L. A. ^{[7
]}

von Braun, K. ^{[8
]}

Youdin, A. ^{[9
]}

机构：

[1] Amer Museum Nat Hist, Dept Astrophys, New York, NY 10024 USA

[2] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA

[3] Univ Hawaii, Dept Geol & Geophys, Honolulu, HI 96822 USA

[4] UJF Grenoble 1, CNRS, INSU, IPAG,UMR 5274, F-38041 Grenoble, France

[5] Univ St Andrews, Sch Phys & Astron, SUPA, St Andrews KY16 9SS, Fife, Scotland

[6] Georgia State Univ, Dept Phys & Astron, Atlanta, GA 30302 USA

[7] MIT, Dept Phys, Cambridge, MA 02139 USA

[8] CALTECH, NASA Exoplanet Sci Inst, Pasadena, CA 91125 USA

[9] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

来源：

ASTRONOMISCHE NACHRICHTEN | 2013年 / 334卷 / 1-2期

基金：

美国国家科学基金会;

关键词：

stars: planetary systems; stars: late-type; stars: fundamental parameters; EXTRASOLAR GIANT PLANETS; DISK TURBULENCE DRIVEN; LOW-MASS STARS; BROWN DWARFS; GRAVITATIONAL-INSTABILITY; ASTROPHYSICAL PARAMETERS; PLANETESIMAL FORMATION; STREAMING INSTABILITY; PHYSICAL-PROPERTIES; MODEL ATMOSPHERES;

D O I：

10.1002/asna.201211760

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a brief overview of a splinter session on M dwarf stars as planet hosts that was organized as part of the Cool Stars 17 conference. The session was devoted to reviewing our current knowledge of M dwarf stars and exoplanets in order to prepare for current and future exoplanet searches focusing in low mass stars. We review the observational and theoretical challenges to characterize M dwarf stars and the importance of accurate fundamental parameters for the proper characterization of their exoplanets and our understanding on planet formation. (C) 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

引用

页码：155 / 158

页数：4

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