Hostname: page-component-78c5997874-lj6df Total loading time: 0 Render date: 2024-11-07T22:33:15.906Z Has data issue: false hasContentIssue false
  • English
  • Français

Is the Outburst of U Scorpii an Accretion Event?

Published online by Cambridge University Press:  12 April 2016

R.F. Webbink
R.F. Webbink*
Affiliation:
Department of Astronomy, University of Illinois

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.

A summary of the peculiarities of the spectral evolution of the recurrent nova T Cr B are given, and interpreted in terms of an episodic accretion model. On the basis of the marked similarity of U Sco with this nova, it is suggested that the observed maximum will be followed by a secondary maximum, reaching V = 14-15. Such a secondary maximum should be very different for an accretion event (showing a strong continuum) and a thermonuclear outburst (showing a nebular spectrum). If observations of a star at 14th magnitude at the position of U Sco in February 1969 were indeed of a secondary maximum of this nova, the principal maximum probably precedes the secondary by less than 65 days.

Type
Abstracts of Workshop Papers on Novae
Information
International Astronomical Union Colloquium , Volume 53: White Dwarfs and Variable Degenerate Stars , August 1979 , pp. 534
Copyright
Copyright © The University of Rochester 1979