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IUE and Optical Spectra of RZ LMI and ER UMa Throughout their 19 and 43 Day Cycles
Published online by Cambridge University Press: 12 April 2016
Abstract
IUE and optical data were obtained throughout the supercycles of RZ LMi and ER UMa during 1993/94. While most of the spectral and photometric characteristics are consistent with disk changes in systems with a relatively high accretion rate and low inclination, the cause of the high accretion rate in this subset of SU UMa stars is not known.
- Type
- Non-Magnetic Cataclysmic Variables
- Information
- International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 55 - 58
- Copyright
- Copyright © Kluwer 1996