New observations of pulsed X-ray emission from NP 0532

Details New observations of pulsed X-ray emission from NP 0532 New observations of pulsed X-ray emission from NP 0532

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...203l..57k&link_type=abstract

Astrophysical Journal, vol. 203, Jan. 15, 1976, pt. 2, p. L57-L61.

Astronomy and Astrophysics

Astronomy

20

Pulsars, Pulsed Radiation, X Ray Astronomy, X Ray Sources, Pulse Amplitude, Pulse Duration, Statistical Distributions

Scientific paper

Large-area proportional counters sensitive from 0.6 to 23 keV were used to observe about 3 min of pulsed X-ray emission from NP 0532 during two lunar-occultation experiments. A detailed pulse profile with 65-microsec resolution shows that the X-ray primary-pulse shape is essentially identical to its optical counterpart. Spectral data on the pulsed X-ray emission are presented. A pulse-by-pulse examination of the data shows no evidence for temporal variability.

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