Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...143..267b&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 143, no. 2, Feb. 1985, p. 267-273. Research supported by the Nederlandse Organ
Astronomy and Astrophysics
Astronomy
73
Cos-B Satellite, Galactic Cosmic Rays, Galactic Nuclei, Gamma Ray Astronomy, Milky Way Galaxy, Molecular Clouds, Abundance, Carbon Monoxide, Gamma Ray Spectra, Hydrogen Clouds, Interstellar Chemistry, Interstellar Matter
Scientific paper
The gamma-ray flux (E greater than 300 MeV) from the central few hundred parsecs of the Milky Way is shown to be nearly an order of magnitude smaller than the value expected from the H2 masses generally estimated to be present in the center and from the average gamma-ray emissivity measured for the disk. This result implies that in the Galactic center the gamma-ray emissivity is anomalously low, or that molecular hydrogen is nearly an order of magnitude less abundant than estimates made from CO observations. The former suggests that the density of cosmic-ray nuclei with energies of 1 GeV is anomalously small relative to the local value, or perhaps that these cosmic rays do not efficiently penetrate the molecular clouds in the central region of the Galaxy. The latter suggests that the gas-to-dust ratio is anomalously low and that the 3-sigma upper limit to the mass of the nuclear disk is 5.8 x 10 to the 7th solar mass. Circumstantial evidence favors a low H2/CO abundance as the source of the gamma-ray deficiency.
Bania Thomas M.
Blitz Leo
Bloemen Johannes Bernardus Gerhardus Maria
Hermsen Willem
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