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Timing and spectral Properties of PSR B1509–58 observed with BeppoSAX

Published online by Cambridge University Press:  12 April 2016

G. Cusumano ,
T. Mineo ,
L. Nicastro ,
E. Massaro ,
S. Massaglia ,
E. Trussoni  and
W. Becker
G. Cusumano
Affiliation:
Istituto di Fisica Cosmica e Appl. Informatica, CNR, Palermo, Italy
T. Mineo
Affiliation:
Istituto di Fisica Cosmica e Appl. Informatica, CNR, Palermo, Italy
L. Nicastro
Affiliation:
Istituto di Fisica Cosmica e Appl. Informatica, CNR, Palermo, Italy
E. Massaro
Affiliation:
Istituto Astronomico, Università ”La Sapienza”, Roma, Italy
S. Massaglia
Affiliation:
Osservatorio Astronomico di Torino, I-10025 Pino Torinese, Italy
E. Trussoni
Affiliation:
Osservatorio Astronomico di Torino, I-10025 Pino Torinese, Italy
W. Becker
Affiliation:
MPI für Extraterrestrische Physik, Garching bei München, Germany

Abstract

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We present some preliminary results of a BeppoSAX observation of the pulsar PSR B1509–58. We discuss in detail the spectrum energy distribution and show that the high energy data can be explained by a steepening continuum spectrum.

Type
Part 5. High-Energy Observations
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 329 - 330
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

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