Abstract
The mysterious secondary component of ɛ Aur is probably not in a prestellar stage of evolution. It is more likely to be a black hole—a collapsar—formed by a stellar implosion.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Kuiper, G. P., Struve, O., and Stromgren, B., Astrophys. J., 86, 570 (1937).
Kopal, Z., Mem. Soc. Roy. Sci. Liège, 15, 241 (1955).
Kraft, R. D., Astrophys. J., 120, 391 (1954).
Ludendorff, H., Sitzungsber. d. Pruess. Akad. Wiss. (Math.-Naturwiss. Klasse), 9, 49 (1924).
Schoenberg, E., and Jung, B., Astron. Nachr., 265, 221 (1938).
Ezer, D., and Cameron, A. G. W., Canad. J. Phys., 45, 3429 (1967).
Cameron, A. G. W., in Low Luminosity Stars (edit. by Kumar, S. S.) (Gordon and Breach, New York, 1969).
Cameron, A. G. W., EOS, Trans. Amer. Geophys. Union, 51, 628 (1970).
Wilson, J. R., UCRL Report 72363 (1970).
Arnett, W. D., Astrophys. Space Sci., 5, 180 (1969).
Morris, S. C., J. Roy. Astron. Soc. Canad., 56, 210 (1962).
Mitchell, R. I., Astrophys. J., 140, 1607 (1964).
Robertson, H. P., Mon. Not. Roy. Astron. Soc., 97, 423 (1937).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
CAMERON, A. Evidence for a Collapsar in the Binary System ɛ Aur. Nature 229, 178–180 (1971). https://doi.org/10.1038/229178a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/229178a0
This article is cited by
-
Infrared images of the transiting disk in the ε Aurigae system
Nature (2010)
-
An accretion disc surrounding a component of epsilon aurigae
Astrophysics and Space Science (1986)
-
Epsilon Aurigae in eclipse: The light and colour variations
Astrophysics and Space Science (1986)
-
Geometrical and physical elements of four ? Lyrae type eclipsing variables
Astrophysics and Space Science (1985)
-
IUE observations of the eclipsing binary Epsilon Aurigae
Nature (1978)
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.