Observations of accreting pulsars

Details Observations of accreting pulsars Observations of accreting pulsars

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aipc..308..235p&link_type=abstract

The Evolution of X-ray Binaries, Proceedings of a conference held in College Park, MD, 1993. Edited by Steve Holt and Charles S

Astronomy and Astrophysics

Astronomy

15

Emission Spectra, Gamma Ray Astronomy, Gamma Ray Spectra, Neutron Stars, Orbital Elements, Pulsars, Stellar Evolution, Stellar Mass Accretion, X Ray Binaries, X Ray Spectra, Gamma Ray Observatory, Magnetic Fields, Satellite-Borne Instruments, Stellar Winds, Torque

Scientific paper

We discuss recent observations of accreting binary pulsars with the all-sky BATSE instrument on the Compton Gamma Ray Observatory. BATSE has detected and studied nearly half of the known accreting pulsar systems. Continuous timing studies over a two-year period have yielded accurate orbital parameters for 9 of these systems, as well as new insights into long-term accretion torque histories.

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