High spectral resolution observations of the H2 2.12 micron line in Herbig-Haro objects

Details High spectral resolution observations of the H2 2.12 micron line in Herbig-Haro objects High spectral resolution observations of the H2 2.12 micron line in Herbig-Haro objects

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988stin...8925085z&link_type=abstract

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Physics

Fabry-Perot Interferometers, Herbig-Haro Objects, Hydrogen Atoms, Stellar Spectra, B Stars, Infrared Stars, Jet Flow, Shock Waves, Stellar Radiation

Scientific paper

The UKIRT Fabry Perot system was used to obtain high spectral resolution line profiles (30 to 35 km/s) for Herbig Haro objects. The important mechanisms for the H2 emission include shock heating of external molecular gas in the wings of the bow shock associated with the working surface of a high velocity jet, and shock heating of external molecular gas entrained in the flow by internal shocks occurring in the jet itself and or in its boundary layer.

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