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Pulsar spectra analysis

Published online by Cambridge University Press:  12 April 2016

Olaf Maron ,
Jaroslaw Kijak ,
Michael Kramer  and
Richard Wielebinski
Olaf Maron
Affiliation:
J. Kepler Astronomical Center, Pedagogical University, Lubuska 2, PL-65-265 Zielona Góra, Poland
Jaroslaw Kijak
Affiliation:
J. Kepler Astronomical Center, Pedagogical University, Lubuska 2, PL-65-265 Zielona Góra, Poland
Michael Kramer
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
Richard Wielebinski
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany

Abstract

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We have extended the database of flux density measurements of 280 pulsars made by Lorimer et al. (1995) to frequencies higher than 1.4 GHz and lower than 300 MHz. Our analysis shows that the spectral behaviour of the majority of pulsars can be well described by a simple power law (S ~ υα where = −1.8) though some pulsar spectra are described by a ”broken power law” with a break at high frequencies υb ~ 1.8 GHz.

Type
Part 3. Studies of Radio Emission
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 227 - 228
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

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