Ref: ASTROimport-222

Molecular Hydrogen in Star-forming Regions: Implementation of its Microphysics in CLOUDY

Shaw, G. ; Ferland, G. J. ; Abel, N. P. ; Stancil, P. C. ; van Hoof, P. A. M.

published in The Astrophysical Journal, 624, pp. 794-807 (2005)

Abstract: Much of the baryonic matter in the universe is in the form of H2, which includes most of the gas in Galactic and extragalactic interstellar clouds. Molecular hydrogen plays a significant role in establishing the thermal balance in many astrophysical environments and can be important as a spectral diagnostic of the gas. Modeling and interpretation of observations of such environments requires a quantitatively complete and accurate treatment of H2. Using this microphysical model of H2, we present illustrative calculations of prototypical astrophysical environments. This work forms the foundation for future investigations of these and other environments in which H2 is an important constituent.

DOI: 10.1086/429215
Links: link

The record appears in these collections:
Royal Observatory of Belgium > Astronomy & Astrophysics
Science Articles > Peer Reviewed Articles

 Record created 2016-07-01, last modified 2016-07-01