Dust and Molecular Emission from the S235 Star Forming Region

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dc.creatorLee, Jeong-Eun
dc.creatorYoung, Chadwick H.
dc.creatorShirley, Yancy L.
dc.creatorMueller, Kaisa E.
dc.creatorEvans II, Neal J.
dc.date2001-11-05
dc.date.accessioned2026-07-07T10:31:09Z
dc.date.available2026-07-07T10:31:09Z
dc.descriptionWe 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.
dc.description2 pages to appear in Hot Star Workshop III: The Earliest Phases of Massive Star Birth, ASP Conference Series, 2002, ed. P.A. Crowther
dc.identifierhttps://arxiv.org/abs/astro-ph/0111102
dc.identifierhttp://arxiv.org/abs/astro-ph/0111102
dc.identifierASPConf.Ser.267:377-378,2002
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178316
dc.subjectAstrophysics
dc.titleDust and Molecular Emission from the S235 Star Forming Region
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