IUE and Optical Spectra of RZ LMI and ER UMa Throughout their 19 and 43 Day Cycles

Paula Szkody, Andrew Silber, R. K. Honeycutt, J. W. Robertson, D. W. Hoard, Lora Pastwick
1996 International Astronomical Union Colloquium  
AbstractIUE 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.
doi:10.1017/s0252921100038197 fatcat:zy6vezulpfgwna4faw2hbkuknm