Collapsars, Infrared Disks and Invisible Secondaries of Massive Binary Systems

Details Collapsars, Infrared Disks and Invisible Secondaries of Massive Binary Systems Collapsars, Infrared Disks and Invisible Secondaries of Massive Binary Systems

Jan 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971natur.229..180s&link_type=abstract

Nature, Volume 229, Issue 5281, pp. 180-183 (1971).

Physics

22

Scientific paper

The supergiant primary of the eclipsing binary system ɛ Aur is probably a star of high mass burning helium in its core. Cameron's suggestion that the invisible secondary is a massive collapsar surrounded by a cool disk of solid particles is thus given further support. A similar object with a disk may be in orbit around the supergiant 89 Her, which has a large infrared excess of unknown origin. The disk could be formed during the initial stage of collapse of the secondary.

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