Hostname: page-component-848d4c4894-r5zm4 Total loading time: 0 Render date: 2024-06-15T06:06:14.085Z Has data issue: false hasContentIssue false
  • English
  • Français

Mean, individual pulses and spectrum of Geminga radio emission

Published online by Cambridge University Press:  12 April 2016

V.M. Malofeev  and
O.I. Malov
V.M. Malofeev
Affiliation:
Pushchino Radio Astronomy Observatory, Lebedev Physical Institute, 142292, Pushchino, Moskow reg., Russia
O.I. Malov
Affiliation:
Pushchino Radio Astronomy Observatory, Lebedev Physical Institute, 142292, Pushchino, Moskow reg., Russia

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.

The measurements of profiles at 102, 87, 59 and 40 MHz are presented. Geminga shows unique character of radio emission: the most steep spectrum, the large changes of pulse widths, phases of pulse time of arrival and the presence of giant pulses.

Type
Part 3. Studies of Radio Emission
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 241 - 242
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Malofeev, V.M., Malov, O.I. 1997, Nature, 389, 697.CrossRefGoogle Scholar