Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apjs...83..111w&link_type=abstract
Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 83, no. 1, p. 111-146.
Astronomy and Astrophysics
Astronomy
326
Galactic Bulge, Galactic Structure, Infrared Astronomy, Milky Way Galaxy, Monte Carlo Method, Infrared Astronomy Satellite, Infrared Space Observatory (Iso), Point Sources, Space Infrared Telescope Facility, Stellar Spectrophotometry
Scientific paper
We present a detailed model for the IR point-source sky that comprises geometrically and physically realistic representations of the Galactic disk, bulge, stellar halo, spiral arms (including the 'local arm'), molecular ring, and the extragalactic sky. We represent each of the distinct Galactic components by up to 87 types of Galactic source, each fully characterized by scale heights, space densities, and absolute magnitudes at BVJHK, 12, and 25 microns. The model is guided by a parallel Monte Carlo simulation of the Galaxy at 12 microns. The content of our Galactic source table constitutes a good match to the 12 micron luminosity function in the simulation, as well as to the luminosity functions at V and K. We are able to produce differential and cumulative IR source counts for any bandpass lying fully within the IRAS Low-Resolution Spectrometer's range (7.7-22.7 microns as well as for the IRAS 12 and 25 micron bands. These source counts match the IRAS observations well. The model can be used to predict the character of the point source sky expected for observations from IR space experiments.
Cohen Martin
Schwartz Deborah E.
Volk Kevin
Wainscoat Richard J.
Walker Helen J.
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