Highly supersonic molecular flows in wind-clump boundary layers

Details Highly supersonic molecular flows in wind-clump boundary layers Highly supersonic molecular flows in wind-clump boundary layers

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.216..143m&link_type=abstract

Astrophysics and Space Science, vol. 216, no. 1-2, p. 143-150

Astronomy and Astrophysics

Astrophysics

10

Boundary Layer Flow, Gas Dynamics, Hydrogen, Interstellar Gas, Magnetohydrodynamic Flow, Molecular Gases, Orion Nebula, Planetary Nebulae, Plasma Turbulence, Stellar Models, Stellar Winds, Turbulent Boundary Layer, Viscous Flow, Emission Spectra, Line Spectra, Shock Waves, Stellar Spectra

Scientific paper

The gradual acceleration, through viscous coupling to a wind, of
molecular hydrogen in turbulent boundary layers around obstacle clumps
is proposed to be responsible for the widths of the emission features
with full widths at zero intensity of greater than 100 km/s.

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