Relation of core structure to high velocity outflow in G35.2-0.74 and other molecular clouds

Details Relation of core structure to high velocity outflow in G35.2-0.74 and other molecular clouds Relation of core structure to high velocity outflow in G35.2-0.74 and other molecular clouds

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984stfm.work...91l&link_type=abstract

In Royal Observatory Star Formation Workshop p 91-107 (SEE N85-12809 03-88)

Physics

Free Molecular Flow, Interstellar Chemistry, Interstellar Gas, Molecular Clouds, Stellar Winds, Ammonia, Stellar Evolution, Stellar Mass Ejection

Scientific paper

Difficulties in estimating gas densities within molecular clouds are
discussed, quoting observations of HH objects 24-26; confinement of high
velocity gas flows by ambient cloud material is considered. Observations
of the 400M cloud G35.2-0.74 are summarized.

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