Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-26T04:49:37.204Z Has data issue: false hasContentIssue false
  • English
  • Français

Thermal Radiation from a Radio Pulsar: PSR1055-52

Published online by Cambridge University Press:  04 August 2017

W. Brinkmann  and
H. Ögelman
W. Brinkmann
Affiliation:
Max-Planck-Institut für Physik und Astrophysik, Institut für Extraterrestrische Physik, 8046 Garching, FRG
H. Ögelman
Affiliation:
Max-Planck-Institut für Physik und Astrophysik, Institut für Extraterrestrische Physik, 8046 Garching, FRG

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 radiopulsar PSR1055-52 has been observed now by the Exosat observatory for about 105 sec, thus increasing the previously published data base (Brinkmann et al. 1985) by a factor of two. The pulsar was seen in the low energy telescope (0.04–2 keV) with the thin Lexan and Al/Par filters, but not in the Boron filter or with the ME experiment.

Type
V. Neutron Star Physics
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 458
Copyright
Copyright © Reidel 1987 

References

Brinkmann, W., Ögelman, H., Aschenbach, B. 1985, Sp. Sc. Rev. 40, p. 527.Google Scholar
Cheng, A. F., Helfand, D. J. 1983, Ap. J. 271, p. 271.CrossRefGoogle Scholar
Tsuruta, S. 1985, MPA preprint 183.Google Scholar
Alpar, A. M., Anderson, P W., Pines, D., Shaham, J. 1984, Ap. J. 276, p. 325.CrossRefGoogle Scholar