Gas, dust, high energy particles and star formation in the Galactic Center

Details Gas, dust, high energy particles and star formation in the Galactic Center Gas, dust, high energy particles and star formation in the Galactic Center

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....80..276a&link_type=abstract

Astronomy and Astrophysics, vol. 80, no. 3, Dec. 1979, p. 276-286.

Astronomy and Astrophysics

Astrophysics

13

Cosmic Dust, Cosmic Gases, Cosmic Rays, Galactic Evolution, Galactic Nuclei, Milky Way Galaxy, Star Formation, Far Infrared Radiation, Flux Density, Gamma Rays, Lyman Spectra, Stellar Evolution

Scientific paper

The amount of gas and dust in the Galactic Center is evaluated. The COS-B and SAS-2 gamma-ray observations of the Galactic Center are discussed and limits for the flux of high-energy cosmic rays are derived from them. Consideration is given to low-energy cosmic rays which are indirectly responsible via their interaction of the interstellar matter, for X- and gamma-ray lines observed recently. The rate of star formation is derived for the Galactic Center and found to be about three times the rate in the Solar Neighborhood per unit mass of gas.

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