Radiative Transfer Modeling of the Inner Galaxy

Details Radiative Transfer Modeling of the Inner Galaxy Radiative Transfer Modeling of the Inner Galaxy

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21348501s&link_type=abstract

American Astronomical Society, AAS Meeting #213, #485.01; Bulletin of the American Astronomical Society, Vol. 41, p.455

Astronomy and Astrophysics

Astronomy

Scientific paper

Our team uses modifications of pre-existing PDR codes to determine what kind of spectra we will expect from Inner Galaxy Gas. With the new Herschel data expected to come in 2009, these models will predict Inner Galaxy conditions and will aid in the calculation of the mass inflow toward the central black hole. Primary emission lines studied are the [CII] 168 micron, [NII] 122 micron, [NII] 205 micron and [OI] 63 micron cooling features.

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