BeppoSAX observations of the γ-ray pulsars PSR B0656+14 and PSR B1706-44

Details BeppoSAX observations of the γ-ray pulsars PSR B0656+14 and PSR B1706-44 BeppoSAX observations of the γ-ray pulsars PSR B0656+14 and PSR B1706-44

Oct 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..587..575m&link_type=abstract

GAMMA 2001: Gamma-Ray Astrophysics 2001. AIP Conference Proceedings, Volume 587, pp. 575-579 (2001).

Astronomy and Astrophysics

Astrophysics

Pulsars, X-Ray Sources, X-Ray Bursts, X-Ray, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

The Italian-Dutch satelliet for X-ray astronomy BeppoSAX observed the two γ-ray pulsars PSR B0656+14 and PSR B1706-44 in March 1999. Both sources were detected in the LECS and MECS images. No evidence of modulation with the pulsars' period was found. The X-ray spectrum of PSR B0656+14 is complex and requires a three component model, while that of PSR B1706-44 can be fitted by a single power law. .

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