Hostname: page-component-7bb8b95d7b-w7rtg Total loading time: 0 Render date: 2024-09-30T02:15:38.475Z Has data issue: false hasContentIssue false
  • English
  • Français

Physical processes in Cygnus X-2

Published online by Cambridge University Press:  14 August 2015

Robert E. Wilson
Robert E. Wilson*
Affiliation:
Dept. of Astronomy, University of South Florida, Tampa, Fla., U.S.A.

Extract

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.

In developing models for the point X-ray sources the general aim has been to find a common explanation for all such objects. However, important observational differences have already become apparent among the systems having optical identifications. A close examination of the evidence shows that those with the most certain optical identifications, Scorpio X-1 and Cygnus X-2, have very few features in common and, in fact, the model proposed here for Cyg X-2 can probably be excluded for Sco X-1.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 37: Non-Solar X- and Gamma-Ray Astronomy , 1970 , pp. 242 - 246
Copyright
Copyright © Reidel 1970 

References

[1] Kraft, R. P. and Miller, J. S.: 1969, Astrophys. J. 155, L159.CrossRefGoogle Scholar
[2] Sofia, S., Eichhorn, H. K., and Gatewood, G.: 1969, Astron. J. 74, 20.CrossRefGoogle Scholar
[3] Gatewood, G. and Sofia, S.: 1968, Astrophys. J. 154, L69.CrossRefGoogle Scholar
[4] Sofia, S. and Wilson, R. E.: 1968, Nature 218, 73.Google Scholar
[5] Burbidge, E. M., Lynds, C. R., and Stockton, A. N.: 1967, Astrophys. J. 150, L95.Google Scholar
[6] Kraft, R. P. and Demoulin, M. H.: 1967, Astrophys. J. 150, L183.CrossRefGoogle Scholar
[7] Kristian, J., Sandage, A., and Westphal, J. A.: 1967, Astrophys. J. 150, L99.CrossRefGoogle Scholar
[8] Sofia, S.: 1968, Astrophys. Letters 2, 173.Google Scholar
[9] Peimbert, M., Spinrad, H., Taylor, B. J., and Johnson, H. M.: 1968, Astrophys. J. 151, L93.CrossRefGoogle Scholar
[10] Sklovsky, I. S.: 1967, Astrophys. J. 148, L1.CrossRefGoogle Scholar
[11] Sofia, S.: 1967, Astrophys. J. 149, L59.CrossRefGoogle Scholar
[12] Kopal, Z.: 1959, Close Binary Systems, New York, p. 516.Google Scholar
[13] Krzeminski, W. and Kraft, R. P.: 1964, Astrophys. J. 140, 921.CrossRefGoogle Scholar
[14] Kraft, R. P.: 1964, Astrophys. J. 139, 457.CrossRefGoogle Scholar