H2 profiles of C-type bow shocks

Details H2 profiles of C-type bow shocks H2 profiles of C-type bow shocks

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.245..108s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 245, July 1, 1990, p. 108-118. Research supported by SE

Astronomy and Astrophysics

Astronomy

66

Bow Waves, Emission Spectra, Hydrogen, Molecular Clouds, Shock Waves, Herbig-Haro Objects, Line Shape, Magnetic Field Configurations, Photodissociation, Spectral Line Width

Scientific paper

Emission-line profiles of molecular H are presented from curved C-shocks within molecular clouds. The method used to calculate the line profiles is outlined. The method is demonstrated using combinations of either H2 or H2O dominating the cooling with either a paraboloidal or a hemispherical cap shock. The results are consistent with observed profiles from H2 peaks associated with Herbig-Haro objects, but they are not consistent with the particularly broad H2 lines in OMC-1 and DR21.

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