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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

Paula Szkody ,
Andrew Silber ,
R. K. Honeycutt ,
J. W. Robertson ,
D. W. Hoard  and
Lora Pastwick
Paula Szkody
Affiliation:
Dept. of Astronomy, University of Washington, Seattle, WA 98195, USA
Andrew Silber
Affiliation:
Dept. of Astronomy, University of Washington, Seattle, WA 98195, USA
R. K. Honeycutt
Affiliation:
Astronomy Dept., Indiana U, Bloomington, IN 47405, USA
J. W. Robertson
Affiliation:
Astronomy Dept., Indiana U, Bloomington, IN 47405, USA
D. W. Hoard
Affiliation:
Dept. of Astronomy, University of Washington, Seattle, WA 98195, USA
Lora Pastwick
Affiliation:
Dept. of Astronomy, University of Washington, Seattle, WA 98195, USA

Abstract

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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

References

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