Exploring the stellar properties of M dwarfs with high-resolution spectroscopy from the optical to the near-infrared (vol 620, A180, 2018)

被引：0
作者：
Rajpurohit, A. S. [1 ]
Allard, F. [2 ]
Rajpurohit, S. [3 ]
Sharma, R. [1 ]
Teixeira, G. D. C. [4 ,5 ]
Mousis, O. [6 ]
Kamlesh, R. [7 ]
机构：
[1] Phys Res Lab, Astron & Astrophys Div, Ahmadabad 380009, Gujarat, India
[2] Univ Lyon1, Univ Lyon, ENS Lyon, CNRS,Ctr Rech Astrophys Lyon,UMR5574, F-69007 Lyon, France
[3] Univ Gottingen, Inst Theoret Phys, D-37077 Gottingen, Germany
[4] Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, P-4150762 Porto, Portugal
[5] Univ Porto, Dept Fis & Astron, Fac Ciencias, Rua Campo Alegre, P-4169007 Porto, Portugal
[6] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France
[7] Dipartimento Fis & Astron, Via Gobetti 93-2, I-40131 Bologna, Italy
来源：
ASTRONOMY & ASTROPHYSICS | 2019年 / 622卷
关键词：
stars: fundamental parameters; stars: low-mass; stars: atmospheres; errata; addenda;
D O I：
10.1051/0004-6361/201833500e
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
引用
收藏
页数：1
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