Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-28T18:41:25.012Z Has data issue: false hasContentIssue false
  • English
  • Français

The surface and inner temperatures of magnetars

Published online by Cambridge University Press:  20 March 2013

Z. F. Gao ,
N. Wang  and
Q. H. Peng
Z. F. Gao
Affiliation:
Xinjiang Astronomical Observatory, CAS, 150, Science 1-Street, Urumqi Xinjiang, 830011, China email: [email protected]
N. Wang
Affiliation:
Xinjiang Astronomical Observatory, CAS, 150, Science 1-Street, Urumqi Xinjiang, 830011, China email: [email protected]
Q. H. Peng
Affiliation:
Shchool of Astronomy and Space Science, Nanjing University, Nanjing Jiangshu, 210093, China email: [email protected]
Rights & Permissions [Opens in a new window]

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.

Assuming that the timescale of the magnetic field decay is approximately equal to that of the stellar cooling via neutrino emission, we obtain a one-to-one relationship between the effective surface thermal temperature and the inner temperature. The ratio of the effective neutrino luminosity to the effective X-ray luminosity decreases with decaying magnetic field.

Keywords

Magnetarneutrino luminositysurface thermal temperatureinner temperature
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 386 - 388
Copyright
Copyright © International Astronomical Union 2013

References

Du, Y. J., Xu, R. X., Qiao, G. J., & Han, J. L. 2009, MNRAS, 399, 1587Google Scholar
Gao, Z. F., Wang, N., Yuan, J. P., Jiang, L., & Song, D. L. 2011, ApSS, 332, 129Google Scholar
Gao, Z. F., Peng, Q. H., Wang, N., Chou, C.-K., & Huo, W. S. 2011, ApSS, 336, 427Google Scholar
Gao, Z. F., Peng, Q. H., Wang, N., & Chou, C.-K. 2012, Chinese Physics B, Vol. 21. 5, 57109CrossRefGoogle Scholar
Gao, Z. F., Peng, Q. H., Wang, N., & Chou, C.-K. 2012, ApSS, 342, 55Google Scholar
Xu, R. X. 2005, MNRAS, 356, 359Google Scholar
Yakovlev, D. G. & Pethick, C. J. 2004, ARAA 42, 169CrossRefGoogle Scholar