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Observations of millisecond pulsars at 102 MHz

Published online by Cambridge University Press:  12 April 2016

Arkady Kuzmin  and
Boris Losovsky
Arkady Kuzmin
Affiliation:
Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute, Pushchino, Moscow Reg., 142292, Russia
Boris Losovsky
Affiliation:
Pushchino Radio Astronomy Observatory, Astro Space Center, Lebedev Physical Institute, Pushchino, Moscow Reg., 142292, Russia

Abstract

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Millisecond pulsars are differ to ”normal” ones in much weaker frequency dependence of the width of integrated profiles and the absence of the low-frequency turn-over in pulsar spectra.

Type
Part 3. Studies of Radio Emission
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 235 - 236
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Kuzmin, A.D. & Izvekova, V.A., 1993, 260, 724 Google Scholar
Kuzmin, A.D. & Losovsky, B.Ya. 1999a, Astronomy Letters, 25, 375 Google Scholar
Kuzmin, A.D. 1999, ASP Conferene Series, this volumeGoogle Scholar
Kuzmin, A.D. & Losovsky, B.Ya. 1999b, A&A, 352, 489 Google Scholar
Kuzmin, A.D. &. Losovsky, B.Ya. 2000, Astronomy Letters, in pressGoogle Scholar