Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-25T15:42:46.506Z Has data issue: false hasContentIssue false
  • English
  • Français

Observational Manifestations of Young Neutron Stars: Spin-powered Pulsars

Published online by Cambridge University Press:  19 July 2016

Michael Kramer
Michael Kramer*
Affiliation:
University of Manchester, Jodrell Bank Observatory, UK

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 largest number of known young neutron stars axe observed as spin-powered pulsars. While the majority of those are detected at radio frequencies, an increasing number can be studied in other parts of the electromagnetic spectrum as well. The Crab pulsar is the prototype of a young pulsar which can be observed from radio to gamma-ray frequencies, providing a red thread of discussion during a tour through the pulsar properties observed across the electromagnetic spectrum. The basic observational features of pulsar emission are presented, preparing the ground for more detailed reviews given in these proceedings. Here, particular attention will be paid to those emission features which may provide a link between the radio and high-energy emission processes.

Type
Part 1: Neutron Star Formation and Evolution
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 13 - 20
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Becker, W., & Aschenbach, B. 2002, in MPE Rep. 278, Neutron Stars, Pulsars, and Supernova Remnants, eds. Becker, W., Lesch, H., & Trümper, J., (Garching: MPE), p. 64.Google Scholar
Becker, W., & Triimper, J. 1997, A&A, 326, 682.Google Scholar
Brisken, W. F., et al. 2003, ApJ, 593, L89.Google Scholar
Cheng, K. S., Ho, C., & Ruderman, M. 1986, ApJ, 300, 500.Google Scholar
Cordes, J. M. 1978, ApJ, 222, 1006.Google Scholar
Daugherty, J. K., & Harding, A. K. 1996, ApJ, 458, 278.Google Scholar
Gotthelf, E. V., et al. 2000, ApJ, 542, L37.CrossRefGoogle Scholar
Hankins, T. H., et al. 2003, Nature, 422, 141.Google Scholar
Johnston, S., & Romani, R. W. 2003, ApJ, 590, L95.CrossRefGoogle Scholar
Kanbach, G. 2002, in MPE Rep. 278, Neutron Stars, Pulsars, and Supernova Remnants, eds. Becker, W., Lesch, H., & Trümper, J., (Garching: MPE), p. 91.Google Scholar
Kanbach, G., et al. 2003, in Proc. of the SPIE, Instrument Design and Performance for Optical/Infrared Ground-based Telescopes, eds. Masanori, I., & Moorwood, A., 4841, p. 82.Google Scholar
Kramer, M., et al. 1996, A&A, 306, 867.Google Scholar
Kramer, M., et al. 1997, A&A, 322, 846.Google Scholar
Kramer, M., et al. 1998, ApJ, 501, 270.Google Scholar
Kramer, M., et al. 2003a, MNRAS, 342, 1299.Google Scholar
Kramer, M., et al. 2003b, ApJ, 593, L31.Google Scholar
Maron, O., et al. 2000, A&AS, 147, 195.Google Scholar
McLaughlin, M. A., et al. 1996, ApJ, 473, 763.Google Scholar
McLaughlin, M. A., et al. 2003, ApJ, 591, L135.Google Scholar
Migliazzo, J. M., et al. 2002, ApJ, 567, L141.Google Scholar
Moffett, D. A., & Hankins, T. H. 1996, ApJ, 468, 779.CrossRefGoogle Scholar
Morris, D., et al. 1997, A&A, 322, L17.Google Scholar
Murray, S. S., et al. 2002, ApJ, 568, 226.Google Scholar
Possenti, A., et al. 2002, A&A, 387, 993.Google Scholar
Radhakrishnan, V., & Cooke, D. J. 1969, Astrophys. Lett., 3, 225.Google Scholar
Romani, R. W. 1996, ApJ, 470, 469.Google Scholar
Romani, R. W., et al. 2001, ApJ, 563, 221.Google Scholar
Shearer, A., & Golden, A. 2002, in MPE Rep. 278, Neutron Stars, Pulsars, and Supernova Remnants, eds. Becker, W., Lesch, H., & Trümper, J., (Garching: MPE), p. 44.Google Scholar
Shearer, A., et al. 2003, 301, 493.Google Scholar
Thompson, D. J. 2001, in AIP Conf. Proc., Vol. 558, High Energy Gamma-Ray Astronomy, eds. Aharonian, F. A., & Völk, H. J., (New York: AIP), p. 103.Google Scholar
Zhang, B., & Harding, A. K. 2000, ApJ, 535, L51.Google Scholar
Zhang, W., et al. 2001, ApJ, 554, L177.CrossRefGoogle Scholar