Radio emission from RASS sources south of Taurus-Auriga
Astrophysics
2007-05-23 v1
Abstract
We present a 8.4 GHz VLA survey of 50 optical counterparts to 46 ROSAT All-Sky survey (RASS) X-ray sources south of the Taurus-Auriga star-forming region. This survey detected 3 sources with a sensitivity limit of ~ 0.12 mJy. Merging our sample with other radio observations of sources in and around Taurus-Auriga, we find scarce radio emission among RASS sources south of the Taurus-Auriga molecular clouds. Our data support the evidence that these sources are older than weak-lined T Tauri stars, most of them probably being close to the ZAMS.
Keywords
Cite
@article{arxiv.astro-ph/9903125,
title = {Radio emission from RASS sources south of Taurus-Auriga},
author = {A. Magazzu and G. Umana and E. L. Martin},
journal= {arXiv preprint arXiv:astro-ph/9903125},
year = {2007}
}
Comments
6 pages, 2 figures, aa.cls LaTeX class