Computer Science – Sound
Scientific paper
Jan 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21332404l&link_type=abstract
American Astronomical Society, AAS Meeting #213, #324.04; Bulletin of the American Astronomical Society, Vol. 41, p.380
Computer Science
Sound
Scientific paper
Molecular fluorescence is a direct probe of the interaction between the radiation field and molecular gas, and can serve as a sensitive diagnostic tool for the composition, energy transport, and excitation mechanisms in the interstellar medium. I will present aspects of far-ultraviolet molecular fluorescence modeling, together with specific results derived from HST, FUSE, and HUT observations of cometary comae, planetary atmospheres, and planetary nebulae. Future directions include connections between extinction and scattering properties of molecular gas and dust, based on sounding rocket observations of hot young stars and surrounding material, as well as optical and infrared follow-ups.
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