Stellar collapse, pulsars, and globular clusters

Details Stellar collapse, pulsars, and globular clusters Stellar collapse, pulsars, and globular clusters

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...128l...1k&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 128, no. 1, Nov. 1983, p. L1, L2.

Astronomy and Astrophysics

Astrophysics

16

Globular Clusters, Gravitational Collapse, Pulsars, Stellar Evolution, X Ray Sources, Neutron Stars, Stellar Winds, Supernova Remnants

Scientific paper

It is suggested that the discrepancy apparent in the fact that the X-ray and radio pulsar 4U1510-59 has a characteristic age that is several times shorter than its associated SNR, MSH 15-52, may be resolved if the neutron star was formed quietly and the remnant was formed by a relativistic wind, rather than a debris shell. It is noted that the hypothesis that 4U1510-59 may be a member of a class of objects which encompasses PSR0820+02, and the globular cluster X-ray sources, leads to verifiable predictions concerning the proper motion of these objects, as well as of globular cluster dynamics.

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