On the gamma-ray source CG 195 plus 4 /Geminga/

Details On the gamma-ray source CG 195 plus 4 /Geminga/ On the gamma-ray source CG 195 plus 4 /Geminga/

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26a....61l..11m&link_type=abstract

Astronomy and Astrophysics, vol. 61, no. 2, Oct. 1977, p. L11-L13.

Astronomy and Astrophysics

Astronomy

13

Gamma Ray Astronomy, Neutron Stars, Stellar Rotation, Magnetic Moments, Pulsars, Spaceborne Astronomy, Stellar Mass Accretion

Scientific paper

Two different pictures of the pulsating gamma-ray source CG 195 plus 4 observed by the SAS 2 and COS B satellites are discussed. In the former a slowly rotating accreting neutron star surrounded by a cloud thick to X-rays is considered. In the latter the source is supposed to be a freely precessing neutron star with a spin period close to that of MP 0833 and a magnetic moment of 10 to the 31st power G-cu cm. The observations which can be important for clarifying the nature of the source are briefly examined.

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