Deep radio synthesis images of globular clusters

Details Deep radio synthesis images of globular clusters Deep radio synthesis images of globular clusters

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...363l...5k&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 363, Nov. 1, 1990, p. L5-L8. Research supported by the Alfred P.

Astronomy and Astrophysics

Astronomy

35

Binary Stars, Globular Clusters, Pulsars, Radio Astronomy, Astronomical Models, Imaging Techniques, Main Sequence Stars, Stellar Luminosity

Scientific paper

Results are reported from a program of high-resolution and high-sensitivity imaging of globular clusters at 20 cm. The findings indicate that there is not a large number of pulsars in compact binaries which have escaped detection in single-dish pulse searches. Such binaries have been postulated to result from tidal captures of single main-sequence stars. It is suggested that most tidal captures involving neutron stars ultimately result in the formation of a spun-up single pulsar and the complete disruption of the main-sequence star.

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