H2 formation and excitation in diffuse molecular gas

Details H2 formation and excitation in diffuse molecular gas H2 formation and excitation in diffuse molecular gas

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..348..442g&link_type=abstract

Astrophysics in the Far Ultraviolet: Five Years of Discovery with FUSE ASP Conference Series, Vol. 348, Proceedings of the Confe

Astronomy and Astrophysics

Astrophysics

Scientific paper

H2 formation rate and excitation are derived in diffuse molecular clouds from FUSE H2 column densities by using a model of chemical and thermal balance in photon-illuminated interstellar gas. The formation rate appears to be relatively constant and the H2 excitation evidences the existence of a warm component of collisionally excited gas within the molecular gas.

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