HST and Optical Data Reveal White Dwarf Cooling, Spin, and Periodicities in GW Librae 3-4 Years After Outburst

Abstract
Description
Keywords
binaries: close, binaries: spectroscopic, novae, cataclysmic variables, stars: dwarf novae, stars: individual (GW Lib)
Citation
Szkody, P., et al. (2012): HST and Optical Data Reveal White Dwarf Cooling, Spin, and Periodicities in GW Librae 3-4 Years After Outburst. The Astrophysical Journal, 753(2).