TWO NEW VARIABLE HOT DQ STARS

被引:19
作者
Barlow, B. N. [1 ]
Dunlap, B. H. [1 ]
Rosen, R. [2 ]
Clemens, J. C. [1 ]
机构
[1] Univ N Carolina, Dept Phys & Astron, Chapel Hill, NC 27599 USA
[2] Natl Radio Astron Observ, Green Bank, WV 24944 USA
来源
ASTROPHYSICAL JOURNAL LETTERS | 2008年 / 688卷 / 02期
基金
美国国家科学基金会;
关键词
stars: oscillations; stars: variables: other; white dwarfs;
D O I
10.1086/595584
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
收藏
页码:L95 / L98
页数:4
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