Results from a near infrared search for emission-line stars in the Inner Galaxy: Spectra of new Wolf-Rayet stars

被引:35
作者
Homeier, NL
Blum, RD
Pasquali, A
Conti, PS
Damineli, A
机构
[1] European So Observ, Space Telescope European Coordinating Facil, D-8046 Garching, Germany
[2] Univ Wisconsin, Madison, WI USA
[3] Cerro Tololo Interamer Observ, La Serena, Chile
[4] Univ Colorado, JILA, Boulder, CO USA
[5] Univ Colorado, APS Dept, Boulder, CO 80309 USA
[6] Univ Sao Paulo, IAG, BR-01060970 Sao Paulo, Brazil
关键词
stars : Wolf-Rayet; stars : emission-line; Galaxy : center; Galaxy : stellar content; infrared : stars;
D O I
10.1051/0004-6361:20030989
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present follow-up spectroscopy of emission line candidates detected on near-infrared narrow band images in the inner Galaxy (Homeier et al. 2003). The filters are optimized for the detection of Wolf-Rayet stars and other objects which exhibit emission-lines in the 2 mum region. Approximately three square degrees along the Galactic plane have been analyzed in seven narrow-filters (four emission-lines and three continuum). We have discovered 4 new Wolf-Rayet stars and present coordinates, finding charts, and K-band spectra.
引用
收藏
页码:153 / 159
页数:7
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