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
Multiwavelength Photometry and Hubble Space Telescope Spectroscopy of the Old Nova V842 Centaurus
The instability strip for accreting pulsating white dwarfs as a probe for accretion heating/cooling .
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2010-03-11T03:53:58Z/2010-10-14T20:16:56Z
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 comma Paula, 2011, 'Catching Accreting WDs Moving into Their Instability Strip{s}', 1.0, European Space Agency, https://doi.org/10.5270/esa-oaoo4lq