Potential Protostars in Cloud Cores

Details Potential Protostars in Cloud Cores Potential Protostars in Cloud Cores

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..489h&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 489-490

Astronomy and Astrophysics

Astrophysics

1

Star Formation, Protostars, Formaldehyde

Scientific paper

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.

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