EGRET High-Energy Gamma-Ray Observations of the Vela-Carina Region

Details EGRET High-Energy Gamma-Ray Observations of the Vela-Carina Region EGRET High-Energy Gamma-Ray Observations of the Vela-Carina Region

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...183.0406t&link_type=abstract

American Astronomical Society, 183rd AAS Meeting, #04.06; Bulletin of the American Astronomical Society, Vol. 25, p.1294

Astronomy and Astrophysics

Astronomy

Scientific paper

Observations with the Energetic Gamma Ray Experiment Telescope (EGRET) on the Compton Observatory show that the Vela-Carina region of the galactic plane has two principal sources of E>100 MeV gamma rays: localized sources and diffuse emission from cosmic rays interacting with the interstellar gas. In addition to the Vela and B1055-52 pulsars, a number of unidentified sources are seen, particularly in the longitude range from 284(deg) < l < 320(deg) . Source locations, energy spectra, and time variability information will be presented.

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