Gas Dynamics in the Distruption of Molecular Clouds by Young Massive Stars using BEAR

Details Gas Dynamics in the Distruption of Molecular Clouds by Young Massive Stars using BEAR Gas Dynamics in the Distruption of Molecular Clouds by Young Massive Stars using BEAR

Oct 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..267..397n&link_type=abstract

Hot Star Workshop III: The Earliest Stages of Massive Star Birth. ASP Conference Proceedings, Vol. 267. Edited by Paul A. Crowth

Astronomy and Astrophysics

Astronomy

Scientific paper

Spectro-imaging data on S106 and the Orion Bar were obtained in Br gamma, H2 1-0 S(1) and H2 2-1 S(1) at high spectral resolution. Detailed analysis of the band profiles provided information on the dynamics of the atomic and molecular gas surrounding young massive stars. The gas excitation mechanisms were also studied using the H2 line ratio.

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