Observation of the Crab Pulsar with BeppoSAX: study of the pulse profile and phase resolved spectroscopy

Details Observation of the Crab Pulsar with BeppoSAX: study of the pulse profile and phase resolved spectroscopy Observation of the Crab Pulsar with BeppoSAX: study of the pulse profile and phase resolved spectroscopy

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410..553c&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 553-557 (1997).

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Neutron Stars, Luminosities, Magnitudes, Effective Temperatures, Colors, And Spectral Classification, X-Ray

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The Crab Pulsar (PSR B0531+21) was observed by the four Narrow Field Instruments on board the italian-dutch satellite BeppoSAX in August and September 1996, during the Science Verification Phase. The fine time resolution (15 μs) and the high statistics of the data provided phase histograms of very good quality, well suited for phase resolved spectroscopy over the entire energy band (0.1-300 keV) covered by BeppoSAX. In this contribution we present preliminary results of the phase resolved analysis. Moreover, we also carried out a detailed analysis of the behavior of the P2/P1 ratio with the energy.

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