期刊
ASTRONOMY & ASTROPHYSICS
卷 446, 期 2, 页码 515-523出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20054064
关键词
stars : low-mass; brown dwarfs
We present updated results of spectroscopic follow-up observations of a sample of 45 M dwarf candidates identified by Phan-Bao et al. ( 2003, A&A, 401, 959) based on the DENIS photometry and proper motion measurements. Forty one of these are nearby late-M dwarfs (d < 30 pc) with spectral types ranging from M5.0 to M8.5 computed from the spectral indices. One contaminant is probably an F-G main sequence star reddened by intervening dust and three stars that were not observed have previous classifications as M dwarfs in the literature. In this paper, we identify three M7.5, five M8.0, one M8.5 dwarf and confirm two new M8.0 dwarf members of the 25 pc volume.
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