Is CIR X-1 a runaway binary

Details Is CIR X-1 a runaway binary Is CIR X-1 a runaway binary

Publishing date

Apr 1975

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.254..674c&link_type=abstract

Journals

Nature, vol. 254, Apr. 24, 1975, p. 674-676.

Science

Astronomy and Astrophysics

Field

Astronomy

Additional info 2

51

Additional info 3

Eclipsing Binary Stars, Radio Sources (Astronomy), Supernova Remnants, X Ray Sources, Astronomical Maps, Error Analysis, Microwave Emission, Point Sources, X Ray Stars

Type

Scientific paper

Abstract

It has been suggested by Gott (1972) that in many cases after a supernova explosion in a close binary system the collapsed residue of the explosion may be retained in orbit around the runaway second star. In such a case a binary system with high eccentricity and large space velocity would be obtained. Attention is given to the possibility that the Cir X-1 is such a system. Questions regarding the relation between the Cir X-1 and the recently discovered supernova remnant (SNR) G321.9-0.3 are explored.

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