Two New Variable Hot DQ Stars
arXiv:0810.2140 · doi:10.1086/595584
Abstract
We have discovered periodic variations in the light curves of two hot DQ stars from the Sloan Digital Sky Survey, SDSS J220029.08-074121.5 and SDSS J234843.30-094245.3. These are the second and third variables detected among the hot DQs and confirm the existence of a new class of variable white dwarf stars. The amplitudes of the variations are one half as large as those detected in the first discovered variable, SDSS J142625.71+575218.3, and required high signal-to-noise photometry to detect. The pulse shapes of the stars are not like those of known white dwarf pulsators but are similar to the first hot DQ variable, SDSS J142625.71+575218.3.
Accepted for publication in ApJ Letters (14 pages, 5 figures, 2 tables)
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- Photometric variability in a warm, strongly magnetic DQ white dwarf, SDSS J103655.39+652252.2
- A New Small-Amplitude Variable Hot DQ White Dwarf
- Stark Broadening of Carbon and Oxygen Lines in Hot DQ White Dwarf Stars: Recent Results and Applications
- Follow-up Studies of the Pulsating Magnetic White Dwarf SDSS J142625.71+575218.3
- Follow-up Observations of the Second and Third Known Pulsating Hot DQ White Dwarfs
- Hot C-rich white dwarfs: testing the DB-DQ transition through pulsations
- The OmegaWhite Survey for Short-Period Variable Stars IV: Discovery of the warm DQ white dwarf OW J175358.85-310728.9