Hostname: page-component-76fb5796d-25wd4 Total loading time: 0 Render date: 2024-04-25T16:03:24.063Z Has data issue: false hasContentIssue false
  • English
  • Français

The quest for collapsed/frozen stars in single-line spectroscopic binary systems

Published online by Cambridge University Press:  12 October 2016

Virginia Trimble
Virginia Trimble*
Affiliation:
University of California Irvine, Department of Physics and Astronomy Irvine, California 92697, USA email: vtrimble@uci.edu
Rights & Permissions [Opens in a new window]

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.

Black holes are now commonplace, among the stars, in Galactic centers, and perhaps other places. But within living memory, their very existence was doubted by many, and few chose to look for them. Zeldovich and Guseinov were first, followed by Trimble and Thorne, using a method that would have identified HDE 226868 as a plausible candidate, if it had been in the 1968 catalogue of spectroscopic binaries. That it was not arose from an unhappy accident in the observing program of Daniel M. Popper long before the discovery of X-ray binaries and the identification of Cygnus X-1 with that hot, massive star and its collapsed companion.

Keywords

Black holescollapsed starsCygnus X-1HDE 226868spectroscopic binaries
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S308: The Zeldovich Universe: Genesis and Growth of the Cosmic Web , June 2014 , pp. 38 - 45
Copyright
Copyright © International Astronomical Union 2016 

References

Baade, W. & Zwicky, F. 1934, Proc. USNAS, 20, 254 Google Scholar
Batten, A. H. 1968, Publ. Dom. Ap. Obs. 8, 119 Google Scholar
Batten, A. H. 2014, personal e-mail communication Google Scholar
Bolton, C. T. 1972, Nature 235, 271; Nature Phys. Sci. 240, 124Google Scholar
Bregman, J. et al. 1973, ApJL 186, L117 Google Scholar
Dick, S. J. 2013, Discovery and Classification in Astronomy: Controversy and Consensus, Cambridge Univ. Press Google Scholar
Ewing, A. 1964, Science News Letters 8, 39 (January 18)Google Scholar
Ginzburg, V. L. 1990, ARA&A 20, 1 Google Scholar
Guseinov, O. H. & Zeldovich, Ya. B. 1966, A. Zh 43; 303 Sov. Astr. AJ 10, 251Google Scholar
Hjellming, R. M. 1973, ApJL 182, L29 Google Scholar
Landau, L. 1932, Phys. Z. Sowjetunion 1, 285 Google Scholar
Landau, L. 1938, Nature 141, 333 CrossRefGoogle Scholar
Margon, B. 1973, ApJL 185, L143 Google Scholar
Oppenheimer, J. R. & Snyder, H. 1939, PR 56 455 Google Scholar
Oppenheimer, J. R. & Volkoff, G. 1939, PR 55, 374 Google Scholar
Paczyński, B. 1974, A&A 46, 513 Google Scholar
Popper, C. M. 1950, ApJ 111, 495 Google Scholar
Salpeter, E. E. et al. 1971, ApJ 140, 796 CrossRefGoogle Scholar
Schreier, E. et al. 1971, ApJ 170, 121 Google Scholar
Schwarzschild, K. 1916, Sitzber. Preus. Deut. Akad. Wiss. Berlin, KL Math.-Phys. 189-196 & 424-434Google Scholar
Tananbaum, H. et al. 1972, ApJL 177, L5 Google Scholar
Trimble, V. 1973, A&A 23, 81 Google Scholar
Trimble, V., Rose, W. K., & Weber, J. 1973, MNRAS 162, 1p Google Scholar
Trimble, V. L. & Thorne, K. S. 1969, ApJ 156, 1013 Google Scholar
Webster, V. L. & Murdin, P. 1972, Nature 235, 37 CrossRefGoogle Scholar
Zeldovich, Ya. B. 1964, Sov. Phys. Dokl. 9, 165 Google Scholar
Zeldovich, Ya. B. & Guseinov, O. H. 1966, ApJ 144, 840; Sov. Phys. Dokl. 162, 791Google Scholar
Zeldovich, Ya. B. & Novikov, I. D. 1964b, Sov. Phys. Dokl. 9, 834 Google Scholar
Zeldovich, Ya. B. & Novikov, I. D. 1964, Uspekhi Phys. Nauk. 84, 377 (= 7,763 in translation)CrossRefGoogle Scholar
Zeldovich, Ya. B. & Novikov, I. D. 1965, Uspekhi Phys. Nauk. 86, 447 (= 8,522, in translation)Google Scholar
Zeldovich, Ya. B. & Novikov, I. D. 1966, Nuovo Cimento. I 4, 840 Google Scholar