A Millisecond Pulsar in a 6 Hour Orbit: PSR J0751+1807

Details A Millisecond Pulsar in a 6 Hour Orbit: PSR J0751+1807 A Millisecond Pulsar in a 6 Hour Orbit: PSR J0751+1807

Nov 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...453..419l&link_type=abstract

Astrophysical Journal v.453, p.419

Astronomy and Astrophysics

Astronomy

57

Gamma Rays: Observations, Stars: Pulsars: Individual Alphanumeric: Psr J0751+1807, Stars: Binaries: Close, Stars: Fundamental Parameters, Stars: White Dwarfs

Scientific paper

A 3.48 ms pulsar in a 6.3 hr binary orbit has been discovered in a systematic survey of error boxes around unidentified gamma-ray sources. The spin-down energy of the pulsar is not sufficient to power the estimated γ-ray emission from the putative γ-ray source. The mass function, small orbit, low eccentricity, and large timing age imply that the companion is most likely a 0.12 Msun

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