Constraining the evolution of cataclysmic variables via the masses and accretion rates of their underlying white dwarfs
Enigmatic Recurrent Pulsational Variability of the Accreting White Dwarf EQ Lyn (SDSS J074531.92+453829.6)
GW Lib: a Unique Laboratory for White Dwarf Pulsations
GW Librae: a unique laboratory for pulsations in an accreting white dwarf
HST and Optical Data Reveal White Dwarf Cooling, Spin, and Periodicities in GW Librae 3-4 Years after Outburst
Hubble Space Telescope and Ground-based Observations of V455 Andromedae Post-outburst
Hubble Space Telescope and Optical Data on SDSSJ0804+5103 (EZ Lyn) One Year after Outburst
The instability strip for accreting pulsating white dwarfs as a probe for accretion heating/cooling .
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2011-03-13T05:35:49Z/2011-11-03T23:25:06Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, Szkody et al., 2012, 'An Unprecedented Opportunity to Follow 4 Accreting WDs into the Instabilty Strip', 1.0, European Space Agency, https://doi.org/10.5270/esa-yfucygn