Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-26T21:26:56.649Z Has data issue: false hasContentIssue false
  • English
  • Français

Note on LMC X-4

Published online by Cambridge University Press:  07 August 2017

Tibor J. Herczeg
Tibor J. Herczeg*
Affiliation:
Department of Physics and Astronomy University of Oklahoma Norman, Oklahoma 73019, U.S.A.

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.

Orbital and stellar parameters of the massive X-ray binary LMC X-4 are rediscussed with particular attention to a possible “higher mass” (> 1.4 M⊙) neutron star in the system.

Type
Oral and Contributed Papers
Information
Symposium - International Astronomical Union , Volume 151: Evolutionary Processes in Interacting Binary Stars , 1992 , pp. 445 - 448
Copyright
Copyright © Kluwer 1992 

References

Overview: Rappaport, S., Joss, P. C. in “Accretion Driven Stellar X-ray Sources” (eds. Lewin, W. H. G., Van den Heuvel, E. P. J.), Cambridge U. Press 1983.Google Scholar
Spectroscopy: Chevalier, C., Ilovaisky, S. A., A Ap 59, L9, 1977; Hutchings, J., Crampton, D., Cowley, A., Ap J 225, 548, 1978.Google Scholar
Eclipses: Li, F., Rappaport, S., Epstein, A., Nature 271, 37, 1978; White, N. E., Nature 271, 38, 1978.CrossRefGoogle Scholar
Kelley, R. L. et al. Ap J 264, 568, 1983; Pietch, W. et al., Space Sci. Rev. 40, 371, 1985, see also Pakull, M. et al, Space Sci. Rev. 40, 379, 1985.Google Scholar
Pulsar masses: Wolszczan, A., Nature 350, 688, 1991 (1534 + 12); Ryba, M. F., Taylor, J. H., Ap J 371, 739, 1991 (1855 + 09); Taylor, J. H., Weisberg, J. M., Ap J 345, 434, 1989 (1913 + 16); Prince, T. A. et al, Ap J 374, L41, 1991 (2227 + 11C); Lyne, A. G., Bailes, M., MN, 246, P15, 1990 (2303 + 46).CrossRefGoogle Scholar