Add to ORKGUltraviolet observations using the Solar Blind Channel on the Hubble Space Telescope provide light curves and low resolution spectra of three pulsating white dwarfs in the cataclysmic variables SDSS013132.39-090122.3, SDSSJ161033.64-010223.3 and SDSSJ220553.98+115553.7. The UV light curves show enhanced pulsation amplitudes over those from simultaneous and previous optical photometry, while the UV-optical spectra are fit with white dwarf temperatures near 15,000K. These temperatures place the accreting white dwarfs outside the instability zone for non-interacting DAV white dwarfs and show that the instability strip is complex for accreting white dwarfs
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
The primary white dwarf of the cataclysmic variable SDSS J074531.92+453829.6 was discovered to exhib...
Ultraviolet observations using the Solar Blind Channel on the Hubble Space Telescope provide light c...
Ultraviolet observations using the Solar Blind Channel on the Hubble Space Telescope provide light c...
We have obtained Hubble Space Telescope UV spectra of the white dwarf in GW Lib, the only known non-...
Time-resolved low resolution Hubble Space Telescope ultraviolet spectra together with ground-based o...
Time-resolved low resolution Hubble Space Telescope ultraviolet spectra together with ground-based o...
Time-resolved low resolution Hubble Space Telescope ultraviolet spectra together with ground-based o...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Accreting white dwarfs have recently been shown to exhibit non-radial pulsations similar to their no...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
The primary white dwarf of the cataclysmic variable SDSS J074531.92+453829.6 was discovered to exhib...
Ultraviolet observations using the Solar Blind Channel on the Hubble Space Telescope provide light c...
Ultraviolet observations using the Solar Blind Channel on the Hubble Space Telescope provide light c...
We have obtained Hubble Space Telescope UV spectra of the white dwarf in GW Lib, the only known non-...
Time-resolved low resolution Hubble Space Telescope ultraviolet spectra together with ground-based o...
Time-resolved low resolution Hubble Space Telescope ultraviolet spectra together with ground-based o...
Time-resolved low resolution Hubble Space Telescope ultraviolet spectra together with ground-based o...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Accreting white dwarfs have recently been shown to exhibit non-radial pulsations similar to their no...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
Non-radial pulsations have been identified in a number of accreting white dwarfs in cataclysmic vari...
The primary white dwarf of the cataclysmic variable SDSS J074531.92+453829.6 was discovered to exhib...