Dust and Molecular Emission from the S235 Star Forming Region

Details Dust and Molecular Emission from the S235 Star Forming Region Dust and Molecular Emission from the S235 Star Forming Region

2001-11-05

arxiv.org/abs/astro-ph/0111102v1

ASPConf.Ser.267:377-378,2002

Astronomy and Astrophysics

Astrophysics

2 pages to appear in Hot Star Workshop III: The Earliest Phases of Massive Star Birth, ASP Conference Series, 2002, ed. P.A. C

Scientific paper

We present the results of a multi-faceted study of the high-mass star-forming region S235. With the CalTech Submillimeter Observatory (CSO), we have observed and/or mapped over fifty molecular transitions and 350 micron dust emission in an attempt to learn more about the chemistry, kinematics, and mass distribution within this rich region. We have found two dust cores that are not resolved in our molecular line observations and suggest that one of these is a less evolved star-forming core.

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