HST and Optical Data Reveal White Dwarf Cooling, Spin, and Periodicities in GW Librae 3-4 Years After Outburst
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Date
2012-07-10
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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).