Hostname: page-component-848d4c4894-4rdrl Total loading time: 0 Render date: 2024-07-07T19:25:18.409Z Has data issue: false hasContentIssue false

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

Published online by Cambridge University Press:  12 April 2016

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Brazier, K.T.S., Bertsch, D.L., Fichtel, C.E., et al. 1994, MNRAS, 268, 517 CrossRefGoogle Scholar
Boella, G., Butler, R.C., Perola, G.C., et al. 1997, A&AS 122, 299 Google Scholar
Hartmann, D.H., Brown, L.E., Clayton, D.D., et al. 1993, in Isolated Pulsar, ed. Van Riper, K. A., Epstein, R., & Ho, C. (Cambridge Uni. Press), 405 Google Scholar
Mats, S.M., Ulmer, M.P., Grabelsky, D.A., et al. 1994 ApJ, 434, 288 CrossRefGoogle Scholar
Rots, A.H., Jahoda, K., Macomb, D.J., et al. 1997 ApJ, 501, 749 Google Scholar