New upper limits for pulsed soft X-rays from the VELA pulsar PSR 0833-45

Details New upper limits for pulsed soft X-rays from the VELA pulsar PSR 0833-45 New upper limits for pulsed soft X-rays from the VELA pulsar PSR 0833-45

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....88..309z&link_type=abstract

Astronomy and Astrophysics, vol. 88, no. 3, Aug. 1980, p. 309, 310.

Computer Science

Sound

6

Pulsars, Stellar Spectra, X Ray Sources, Pulsed Radiation, Rocket Sounding, X Ray Spectra

Scientific paper

In January 1977 the pulsar PSR 0833-45 was observed by a rocket
experiment consisting of 12 X-ray paraboloidal collectors. No indication
for pulsed flux could be detected. The new upper limits are considerably
lower than former measurements in the energy band 0.09 to 2 keV.

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