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Potential protostars in cloud cores
Authors:Robert L Hurt  Mary Barsony  Alwyn Wootten
Institution:(1) University of California, Riverside, USA;(2) National Radio Astronomy Observatory, USA
Abstract:We present H2CO observations of young protostar candidates in the Serpens Cloud Core. We find evidence for dense molecular gas in the cores of these objects that is warmer than the surrounding dust. The strong emission and gas properties support the premise that many of these sources may be very young protostars.
Keywords:star formation  protostars  formaldehyde
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