Molecular hydrogen and thermal phases in astrophysics

Details Molecular hydrogen and thermal phases in astrophysics Molecular hydrogen and thermal phases in astrophysics

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phdt.........5l&link_type=abstract

Ph.D. Thesis Colorado Univ., Boulder.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Diatomic Gases, Hydrogen, Interstellar Gas, Molecules, Big Bang Cosmology, Dissociation, Emission Spectra, Molecular Clouds, Quasars, Thermodynamic Properties, X Ray Sources

Scientific paper

The importance of hydrogen molecules (H2) in astrophysics and the connection of atomic and molecular physics with radiative, thermal, and dynamical processes in space are examined. Detailed models of the thermal structure and spectral emission of interstellar gas are constructed for a variety of astrophysical environments; X-ray sources in molecular clouds; quasars; and the early universe.

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