A search for optical millisecond pulsars in globular clusters

Details A search for optical millisecond pulsars in globular clusters A search for optical millisecond pulsars in globular clusters

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...335..753m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 335, Dec. 15, 1988, p. 753, 754. Research sponsored by the Research Corp.,

Astronomy and Astrophysics

Astrophysics

1

Globular Clusters, Pulsars, Pulse Duration, Radio Emission, X Ray Binaries, Neutron Stars, Stellar Luminosity, Stellar Magnetic Fields, Stellar Mass

Scientific paper

A search for millisecond optical pulsars in several bright, compact globular clusters was conducted. The sample included M28, and the X-ray clusters 47 Tuc, NGC 6441, NGC 6624, M22, and M15. The globular cluster M28 contains the recently discovered 327 Hz radio pulsar. Upper limits of 4 sigma to pulsed emission of (1-20) solar luminosities were found for the globular clusters tested, and 0.3 solar luminosity for the M28 pulsar for frequencies up to 500 Hz.

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