High-energy X-ray observations of A0535 + 26

Details High-energy X-ray observations of A0535 + 26 High-energy X-ray observations of A0535 + 26

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.243..475c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 243, April 1, 1990, p. 475-479. Research supported by C

Astronomy and Astrophysics

Astronomy

8

Pulsars, Stellar Mass Accretion, X Ray Astronomy, X Ray Binaries, Balloon-Borne Instruments, Energetic Particles, Stellar Luminosity, Stellar Spectra, X Ray Telescopes

Scientific paper

High-energy X-ray observations of the binary pulsar A0535 + 26 over the photon energy range 26-288 keV were obtained from a flight in July 1986 of the MIFRASO balloon-borne telescope. The source was detected in a low state, and a pulse period of 103.54 s was measured. The results are compared to, and discussed in the context of, other observations over the last 10 years.

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