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X-ray Emission Characteristics of Pulsars

Published online by Cambridge University Press:  25 May 2016

W. Becker*
Affiliation:
Max-Planck-Institut für extraterrestrische Physik, Giessenbachstrasse 1, Postfach 1603, 85740 Garching, Germany

Abstract

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Recent X-ray observatories such as ROSAT, ASCA, RXTE, BeppoSAX, and Chandra have achieved important progress in neutron star and pulsar astronomy. The identification of Geminga as a rotation-powered pulsar, the discovery of X-ray emission from millisecond pulsars, and the identification of cooling neutron stars are only a few of the fascinating results. In the following, I will give a brief review on the X-ray emission properties of rotation-powered pulsars and their wind nebulae.

Type
Part I: Talks
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Becker, W., & Aschenbach, B. 1995, in The Lives of Neutron Stars, eds. Alpar, A., Kilizóglu, U., & van Paradijs, J. (Dordrecht: Kluwer), 47.CrossRefGoogle Scholar
Becker, W., Kawai, N., Brinkmann, W., & Mignani, R. 1999, A&A, 352, 532.Google Scholar
Becker, W., & Trümper, J. 1996, A&AS, 120, C69.Google Scholar
Becker, W., & Trümper, J. 1997, A&A, 326, 682.Google Scholar
Becker, W., & Trümper, J. 1999, A&A, 341, 803.Google Scholar
Brazier, K. T. S., & Becker, W. 1997, MNRAS, 284 335.CrossRefGoogle Scholar
Greiveldinger, C., & Aschenbach, B. 1999, ApJ, 510, 305.CrossRefGoogle Scholar
Greiveldinger, C., et al. 1996, ApJ, 465, L35.CrossRefGoogle Scholar
Gotthelf, E. V., & Kulkarni, S. R. 1997, ApJ, 490, L161.CrossRefGoogle Scholar
Halpern, J. P., & Wang, F. Y.-H. 1997, ApJ, 477, 905.CrossRefGoogle Scholar
Hartman, R. C., et al. 1999, ApJS, 123, 79.CrossRefGoogle Scholar
Kawai, N., & Saito, Y. 1999, in 3rd INTEGRAL Workshop, The Extreme Universe (Sept. 1998, Taormina, Italy), in press.Google Scholar
Kawai, N., & Tamura, K. 1996, in ASP Conf. Ser. Vol. 105, Pulsars: Problems and Progress, eds. Johnston, S., Walker, M. A., & Bailes, M. (San Francisco: ASP), 367.Google Scholar
Kuiper, L., Hermsen, W., Verbunt, F., & Belloni, T. 1998, A&A, 336, 545.Google Scholar
Kuiper, L., et al. 1999, in 3rd INTEGRAL Workshop, The Extreme Universe (Sept. 1998, Taormina, Italy), in press.Google Scholar
Marquart, C.B., & Ögelman, H. 1999, in Workshop on the Relationship Between Neutron Stars and Supernova Remnants, eds. Bandiera, R., Masini, E., Pacini, F., Salvati, M., & Woltjer, L., Mem. Soc. Astron. Italy, 69, no. 4, 927.Google Scholar
Mereghetti, S. 1999, astro-ph/9911252, preprint.Google Scholar
Michel, F. C. 1991, Theory of Neutron Star Magnetospheres (Chicago: University of Chicago Press).Google Scholar
Mineo, T., et al. 2000, A&A, submitted.Google Scholar
Ögelman, H. 1995, The Lives of Neutron Stars, eds. Alpar, A., Kilizóglu, U., & van Paradijs, J. (Dordrecht: Kluwer), 101.CrossRefGoogle Scholar
Ögelman, H., Finley, J.P., & Zimmerman, H. U. 1993, Nature, 361, 136.CrossRefGoogle Scholar
Pavlov, G. G. 2000, these Proceedings.Google Scholar
Safi-Harb, S., Ögelman, H., & Finley, J. P. 1995, ApJ, 439, 722.CrossRefGoogle Scholar
Saito, Y., Kawai, N., Kamae, T., Shibata, S., Dotani, T., & Kulkarni, S. R. 1997, ApJ, 477, L37.CrossRefGoogle Scholar
Seward, F. D., & Wang, Z. R. 1988, ApJ, 332, 199.CrossRefGoogle Scholar
Shibata, S., et al. 1997, ApJ, 483, 843.CrossRefGoogle Scholar
Takahashi, M., Shibata, S., Torii, K., Saito, Y., & Kawai, N. 1998, IAU Circ. 7030.Google Scholar
Tamura, K., Kawai, N., Yoshida, A., & Brinkmann, W. 1996, PASJ, 48, L33.CrossRefGoogle Scholar
Tsuruta, S. 1998, Phys. Rep., 292, 1.CrossRefGoogle Scholar
Ulmer, M. P., et al. 1993, ApJ, 417, 738.CrossRefGoogle Scholar
Verbunt, F., Kuiper, L., Belloni, T., Johnston, H. M., de Bruyn, A. G., Hermsen, W., & van der Klis, M. 1996, A&A, 311, L9.Google Scholar
Wang, Z. R., Li, Z. Y., & Begelman, M. C. 1993, Nature, 364, 127.CrossRefGoogle Scholar
Wang F., Y.-H., Ruderman, M., Halpern, J. P., & Zhu, T. 1998, ApJ, 498, 373.CrossRefGoogle Scholar
Yancopoulos, S., Hamilton, T. T., & Helfand, D. J. 1994, ApJ, 429, 832.CrossRefGoogle Scholar