The dominant 10 to 20 micrometer source in the galactic centre

Details The dominant 10 to 20 micrometer source in the galactic centre The dominant 10 to 20 micrometer source in the galactic centre

Nov 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974hrgc.conf..229b&link_type=abstract

H II regions and the galactic centre : proceedings of the Eighth ESLAB Symposium, 4-7 June 1974, Frascati, Italy, p. 229-233 (SE

Astronomy and Astrophysics

Astronomy

2

Galactic Structure, Infrared Radiation, Radiation Sources, Cosmic Dust, Hydrogen Clouds, Hydrogen Ions, Lyman Alpha Radiation, Protostars, Radio Sources (Astronomy)

Scientific paper

The dominant 10 - 20 microns source in the galactic center is a 4" x 6" object, coinciding with a compact radio source. It is suggested that the radiation is due to dust, which competes efficiently with the hydrogen to capture Lyman-continuum photons, or that the dust is heated by protostars which are just becoming hot enough to start ionizing the hydrogen.

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