Dust and Molecular Emission from the S235 Star Forming Region

Chadwick H. Young; Jeong-Eun Lee; Kaisa E. Mueller; Neal J. Evans II (Department of Astronomy; The University of Texas at Austin); Yancy L. Shirley

arxiv: astro-ph/0111102 · v1 · submitted 2001-11-05 · 🌌 astro-ph

Dust and Molecular Emission from the S235 Star Forming Region

Jeong-Eun Lee , Chadwick H. Young , Yancy L. Shirley , Kaisa E. Mueller , Neal J. Evans II (Department of Astronomy , The University of Texas at Austin) This is my paper

classification 🌌 astro-ph

keywords dustmolecularregionemissions235star-formingattemptcaltech

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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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Dust and Molecular Emission from the S235 Star Forming Region

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