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27 April 2024
 
  » arxiv » astro-ph/9612193

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Search for young low-mass stars in a ROSAT selected sample south of the Taurus-Auriga molecular clouds
A. Magazzu ; E. L. Martin ; M. F. Sterzik ; R. Neuhaeuser ; E. Covino ; J.M. Alcala ;
Date 19 Dec 1996
Journal Astron.Astrophys.Suppl.Ser. 124 (1997) 449
Subject astro-ph
AbstractWe present results of intermediate resolution spectroscopy of 131 optical counterparts to 115 ROSAT All-Sky Survey X-ray sources south of the Taurus-Auriga dark cloud complex. These objects have been selected as candidate young stars from a total of 1084 ROSAT sources in a about 300 square degree area. We identify 30 objects as low-mass PMS stars on the basis of the Li 6708 doublet in their spectrum, a signature of their young age. All these stars have a spectral type later than F7 and show spectral characteristics typical of weak-line and post-T Tauri stars. The presence of young objects several parsecs away from the regions of ongoing star formation is discussed in the light of the current models of T Tauri dispersal.
Source arXiv, astro-ph/9612193
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