Γ-rays from 3C273: scaling the orion cloud complex

Details Γ-rays from 3C273: scaling the orion cloud complex Γ-rays from 3C273: scaling the orion cloud complex

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.200..343s&link_type=abstract

Astrophysics and Space Science, Volume 200, Issue 2, pp.343-345

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Orion cloud complex in the Milky Way is a source ofγ-rays attributable to cosmic-ray interactions with ambient thermal gas. Quantities upon which theγ-ray flux depends can be scaled to the QSO 3C273. This result supports the hypothesis that at least some of theγ-rays from this object and other QSOs may also be attributed to a similarpp-interaction scenario.

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