Molecular Shocks in Star Forming Regions

Details Molecular Shocks in Star Forming Regions Molecular Shocks in Star Forming Regions

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..125b&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 125-138

Astronomy and Astrophysics

Astrophysics

1

Molecular Hydrogen, Shocks, Outflows

Scientific paper

The role of excited molecular hydrogen as a powerful observational tool
is examined in the context of shock phenomena in molecular clouds,
particularly in star forming regions. Conclusions that may be drawn from
line intensities and line profiles, and the properties of J and C shocks
in a bow shock structure are discussed.

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