Two gamma-ray sources and ancient guest stars

Details Two gamma-ray sources and ancient guest stars Two gamma-ray sources and ancient guest stars

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987sci...235.1485w&link_type=abstract

Science (ISSN 0036-8075), vol. 235, March 20, 1987, p. 1485, 1486.

Astronomy and Astrophysics

Astronomy

5

Histories, Neutron Stars, Pulsars, Supernova Remnants, Supernovae, Crab Nebula, Gamma Ray Astronomy, Ophiuchi Clouds

Scientific paper

On the basis of the fact that the youngest neutron stars such as the Crab pulsar and the Vela pulsar emit strong gamma-ray radiation, it is suggested that a few gamma-ray sources may be identified with young compact sources formed in the events of guest stars. Two such sources, 2CG 353 + 16 and 2CG 054 + 01, are identified with guest stars observed in the 14th century B.C. and A.D. 1230, respectively.

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