A flywheel model for CYG X-3 - A case for a strict relation with SCO X-1

Details A flywheel model for CYG X-3 - A case for a strict relation with SCO X-1 A flywheel model for CYG X-3 - A case for a strict relation with SCO X-1

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987mnras.225p..39t&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 225, April 1, 1987, p. 39P-42P.

Astronomy and Astrophysics

Astronomy

6

Flare Stars, Stellar Magnetic Fields, Stellar Mass Accretion, Stellar Models, Stellar Rotation, Emission Spectra, Spectral Energy Distribution, X Ray Spectra

Scientific paper

The authors propose that Cyg X-3 is powered by both accretion and
rotation of a rapidly spinning neutron star endowed of a modest magnetic
field. This makes the system close to Sco X-1 in the description
recently suggested by Priedhorsky. In particular the possibility of
producing the high-energy emission is discussed.

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