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Where is Nova 1437? - Surprises in the Space Density of Cataclysmic Variables
Published online by Cambridge University Press: 12 April 2016
Abstract
A U-B search to 21st magnitude in a 1°×1° region centered on the best position for the Korean nova of 1437 has revealed no unique candidate. Instead, we find 7 faint UV-bright stars with CV-like emission lines. The implied space density is two orders of magnitude higher than the classical space density for CV’s.
- Type
- 1a. Basic Properties of Novae
- Information
- International Astronomical Union Colloquium , Volume 122: Physics of Classical Novae , 1990 , pp. 57 - 58
- Copyright
- Copyright © Springer-Verlag 1990
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