Radio Emission from Young Stellar Objects in the LkH α 101 Region

Details Radio Emission from Young Stellar Objects in the LkH α 101 Region Radio Emission from Young Stellar Objects in the LkH α 101 Region

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aas...191.0512s&link_type=abstract

American Astronomical Society, 191st AAS Meeting, #05.12; Bulletin of the American Astronomical Society, Vol. 29, p.1215

Astronomy and Astrophysics

Astronomy

Scientific paper

We present results of a VLA 3.6 cm B configuration survey of a region around LkH α 101. LK H α 101 is a Herbig Ae/Be star possessing a strong ionized stellar wind and an extended H II region. The star appears as the brightest object in a cluster of very young, highly obscured stars. We detect at least 16 sources down to 5 RMS thresholds of 0.25 mJy, most of which are thought to be associated with the star formation region. Several of the sources exhibit high radio variability, with the 3.6 cm emission varying by factors of 5 on a timescale of hours. One confirmed T Tauri star in the cloud exhibited such variation.

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