EXOSAT observation of the pulsar PSR 1509-58

Details EXOSAT observation of the pulsar PSR 1509-58 EXOSAT observation of the pulsar PSR 1509-58

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..657t&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 657-659 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

Exosat Satellite, Pulsars, Radiant Flux Density, Satellite Imagery, Supernova Remnants, Energy Bands, Pulse Amplitude, Pulse Duration, Radio Frequencies, X Ray Astronomy, X Ray Sources

Scientific paper

The results of an EXOSAT observation of the radio and X ray pulsar PSR 1509-58, associated with the supernova remnant MSH 15-52 are presented. In the energy range 1.5 to 10 keV the radiation flux detected by the medium energy instrument was fitted with a power law. The period of the pulsar was measured with a value of approx. 0.150362 s, in agreement with the value obtained from the low energy data (energy range 0.02 to 2.5 keV), and with extrapolation from previous observations at X and radio frequencies.

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