Ratios of molecular hydrogen line intensities in shocked gas - Evidence for cooling zones

Details Ratios of molecular hydrogen line intensities in shocked gas - Evidence for cooling zones Ratios of molecular hydrogen line intensities in shocked gas - Evidence for cooling zones

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...334l.103b&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 334, Nov. 15, 1988, p. L103-L106.

Astronomy and Astrophysics

Astrophysics

134

Astronomical Spectroscopy, Gas Density, H Lines, Molecular Clouds, Orion Nebula, Shock Wave Propagation, Molecular Rotation, Vibrational Spectra, Wavelengths

Scientific paper

Column densities of molecular hydrogen have been calculated from 19 infrared vibration-rotation and pure rotational line intensities measured at peak 1 of the Orion molecular outflow. The run of column density with energy level is similar to a simple cooling zone model of the line-emitting region, but is not well fitted by predictions of C-shock models current in the literature.

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