Hostname: page-component-5c6d5d7d68-tdptf Total loading time: 0 Render date: 2024-08-15T22:16:19.574Z Has data issue: false hasContentIssue false
  • English
  • Français

Pulsar Observations and Neutron Star Models

Published online by Cambridge University Press:  14 August 2015

Gerhard Börner  and
Jeffrey M. Cohen
Gerhard Börner*
Affiliation:
Laboratory for High Energy Astrophysics, NASA/Goddard Space Flight Center, Greenbelt, Md., U.S.A.
Jeffrey M. Cohen*
Affiliation:
Laboratory for High Energy Astrophysics, NASA/Goddard Space Flight Center, Greenbelt, Md., U.S.A.
*
∗Permanent address: Max-Planck-Institut für Physik und Astrophysik München, Germany and National Academy of Science-NRC Research Associate.
∗∗Permanent address: Physics Department, University of Pennsylvania, Philadelphia, Pennsylvania 19104. National Academy of Science-NRC Senior Research Associate.

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.

Information about the physical parameters of neutron stars is obtained from pulsar observations. The energy balance of the Crab Nebula and the Vela X remnant allows one to derive limits for the masses of the Crab and Vela pulsars. Glitch observations provide further clues on the masses of these two pulsars. The degree of confidence with which one should believe the derived numbers is pointed out. The possibility of observing neutron stars in binary systems as pulsating X-ray sources is discussed. Finally, the importance of observing redshifted gamma ray lines from the surface of neutron stars, and thus directly measuring either individual or statistical properties of these objects, is pointed out.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 53: Physics of Dense Matter , 1974 , pp. 227 - 236
Copyright
Copyright © Reidel 1974 

References

Baldwin, J. E.: 1971, in Davies, R. D. and Smith, F. G. (eds.), ‘The Crab Nebula’, IAU Symp. 46, 22.Google Scholar
Baym, G. and Pines, D.: 1971, A. de Shalit Memorial Volume.Google Scholar
Baym, G., Bethe, H. A., and Pethick, C.: 1972, (to be published).Google Scholar
Baym, G., Pethick, C., and Sutherland, P.: 1971, Astrophys. J. 179, 200.Google Scholar
Bethe, H. A. and Johnson, M.: 1973 (to be published).Google Scholar
Bethe, H. A., Börner, G., and Sato, K.: 1970, Astron. Astrophys. 7, 279.Google Scholar
Biermann, L.: 1972, Boulder Lecture (‘Cosmic Plasma Physics’).Google Scholar
Börner, G. and Cohen, J. M.: 1972, Astron. Astrophys. 19, 109.Google Scholar
Börner, G., Meyer, F., Schmidt, H. U., and Thomas, H. C.: 1972, Contribution to Fall Meeting of the DAG, Wien.Google Scholar
Cohen, J. M. and Cameron, A. G. W.: 1971, Astrophys. Space Sci. 10, 227.Google Scholar
Cohen, J. M., Langer, W. D., Rosen, L. C., and Cameron, A. G. W.: 1970, Astrophys. Space Sci. 6, 228.Google Scholar
Goldreich, P. and Julian, W. H.: 1969, Astrophys. J. 157, 869.Google Scholar
Gunn, J. E. and Ostriker, J. P.: 1969, Astrophys. J. 157, 1395.Google Scholar
Johnson, W. N. III, Harnden, F. R., and Haymes, R. C.: 1972, Astrophys. J. Letters 172, L1.CrossRefGoogle Scholar
Leung, Y. C. and Wang, C. G.: 1971, Astrophys. J. 170, 499.Google Scholar
Manchester, R. N. and Taylor, J. G.: 1972, Astrophys. Letters 10, 67.Google Scholar
Maran, S. P. and Cameron, A. G. W.: 1969, Earth Extraterrestr. Sci. 1, 3.Google Scholar
Milne, D. K.: 1970, Australian J. Phys. 23, 425.Google Scholar
Minkowski, R.: 1968, Stars and Stellar Systems 7, Ch. 11.Google Scholar
Ramaty, R., Börner, G., and Cohen, J. M.: 1972 (to be published).Google Scholar
Schreier, E., Levinson, R., Gursky, H., Kellogg, E., Tananbaum, H., and Giacconi, R.: 1972, Astrophys. J. Letters 172, L79.Google Scholar
Shklovsky, I.: 1967, Astrophys. J. Letters 150, L48.Google Scholar
Tananbaum, H., Gursky, H., Kellogg, E. M., Levinson, E., Schreier, E., and Giacconi, R.: 1972, Astrophys. J. Letters 174, L143.CrossRefGoogle Scholar
Trimble, V.: 1968, Astron. J. 73, 535.Google Scholar
Trimble, V. and Rees, M. J.: 1970, Astrophys. Letters 5, 93.Google Scholar
Trimble, V. and Woltjer, L.: 1971, Astrophys. J. Letters 163, L97.Google Scholar
Tucker, W. H.: 1971, Astrophys. J. Letters 167, L85.Google Scholar
Wallerstein, G. and Silk, J.: 1971, Astrophys. J. 170, 289.Google Scholar
Woltjer, L.: 1958, Bull. Astron. Inst. Neth. 14, 39.Google Scholar