Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-26T06:26:04.333Z Has data issue: false hasContentIssue false
  • English
  • Français

Effect of Photon Rocket in X-ray Binaries

Published online by Cambridge University Press:  12 April 2016

V. D. Pal’shin  and
A. I. Tsygan
V. D. Pal’shin
Affiliation:
Ioffe Physical Technical Institute, Politekhnicheskaya, 26, 194021 St.Petersburg, Russia
A. I. Tsygan
Affiliation:
Ioffe Physical Technical Institute, Politekhnicheskaya, 26, 194021 St.Petersburg, 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.

It is shown that X-ray binaries can be accelerated by their own radiation. It is possible if the magnetic field of a neutron star in a binary differs from the dipolar field. Asymmetric X-ray emission generated due to accretion of matter onto a neutron star surface creates an accelerating force. Its magnitude can be comparable or even larger than gravitational attraction of the binary to the Galaxy.

Type
Part 9. Population and Neutron Star Properties
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 653 - 654
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Carlberg, R.G., & Innanen, K.A. 1987, AJ, 94, 666 Google Scholar
Pal’shin, V. D., & Tsygan, A.I. 1998, Astron. Lett., 24, 131 Google Scholar
van Paradijs, J., & White, N., 1995, ApJ, 447, L33 CrossRefGoogle Scholar