New neighbours - VI. Spectroscopy of DENIS nearby stars candidates

被引:43
作者
Crifo, F [1 ]
Phan-Bao, N
Delfosse, X
Forveille, T
Guibert, J
Martín, EL
Reylé, C
机构
[1] Observ Paris, GEPI, 5 Pl J Janssen, F-92195 Meudon, France
[2] Acad Sinica, Inst Astron & Astrophys, Taipei 106, Taiwan
[3] Univ Grenoble 1, Lab Astrophys Grenoble, F-38041 Grenoble, France
[4] Canada France Hawaii Telescope Corp, Kamuela, HI 96743 USA
[5] Observ Paris, Ctr Anal Images, GEPI, F-75014 Paris, France
[6] Inst Astrofis Canarias, E-38200 San Cristobal la Laguna, Tenerife, Spain
[7] Univ Cent Florida, Dept Phys, Orlando, FL 32816 USA
[8] Univ Hue, Dept Phys, Hue, Vietnam
[9] Observ Besancon, CNRS, UMR 6091, F-25010 Besancon, France
关键词
stars : low-mass; brown dwarfs; solar neighbourhood; stars : fundamental parameters; stars : distances;
D O I
10.1051/0004-6361:20052998
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present spectra of 36 nearby star candidates and 3 red giant candidates, identified in the DENIS database. 32 of the dwarf candidates are nearby red dwarfs, with spectral types from M 5.5 to M 8.5. Out of 11 targets with low proper motion (mu < 0.1 arcsec yr(-1)) but a Reduced Proper Motion above an inclusive threshold, 9 are red dwarfs. The 4 contaminants are all reddened F-K main sequence stars, and could have been eliminated by checking for small well-known high latitude molecular clouds. These stars might be of interest as probes of interstellar absorption. For the red dwarfs we derive spectral types and spectroscopic distances, using a new calibration of the PC3 spectral index to absolute magnitudes in the I, J, H and K photometric bands. We confirm 2 new members of the 12 pc volume (2 new M 8.5), and one M 7.5 NLTT object closer than 10 pc; and show that one quarter of the stars with photometric distances under 30 pc have too small a proper motion for inclusion in the NLTT catalog.
引用
收藏
页码:653 / 661
页数:9
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