Infrared radiation model for the galactic centre

Details Infrared radiation model for the galactic centre Infrared radiation model for the galactic centre

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hrgc.conf..239a&link_type=abstract

H II regions and the galactic centre : proceedings of the Eighth ESLAB Symposium, 4-7 June 1974, Frascati, Italy, p. 239-245 (SE

Astronomy and Astrophysics

Astronomy

Astronomical Models, Galactic Structure, Infrared Astronomy, Interstellar Matter, Milky Way Galaxy, Stellar Radiation, Cosmic Dust, Heating, Infrared Radiation

Scientific paper

A model is discussed which details the general view that the infrared radiation from the galactic center region originates from interstellar dust heated by stellar radiation. Its ingredients are the stellar mass model for the galactic center, and Spinrad's model for the stellar population in the nucleus of M31. A simple theoretical oscillator model is used for the infrared radiative properties of dust particles. Some qualitative remarks are made regarding the treatment and its approximations.

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