Very high energy gamma-ray binary stars

Details Very high energy gamma-ray binary stars Very high energy gamma-ray binary stars

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sci...238.1528l&link_type=abstract

Science (ISSN 0036-8075), vol. 238, Dec. 11, 1987, p. 1528-1534. DOE-supported research.

Astronomy and Astrophysics

Astronomy

15

Gamma Ray Astronomy, X Ray Binaries, Cosmic Rays, Pulsars

Scientific paper

The data on four recently observed very-high-energy gamma-ray binary stars, Hercules X-1, 4U0115+63, Vela X-1, and Cygnus X-3, are reviewed. Models to explain these sources are briefly addressed. The implication of the observations is that a significant portion of the more energetic cosmic rays observed on earth may arise from the action of similar sources within the Galaxy during the past few million years.

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