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HS 2331+3905, the brightest CV white dwarf pulsator

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Gänsicke, B. T. (Boris T.) (2007) HS 2331+3905, the brightest CV white dwarf pulsator. In: 15th European Workshop on White Dwarfs, AUG 07-11, 2006, Univ Leicester, Leicester, ENGLAND.

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Abstract

We report preliminary results of infrared spectroscopy and of a multi-site photometric campaign on the brightest pulsating white dwarf in a cataclysmic variable (CV), HS 2331+ 3905. The Gemini J, H, and K spectra fail to reveal a clear signature of the donor star, constraining its spectral type to be L2 or later. The presence of two short-period signals at 67.62 s and 67.24 s is confirmed, and we identify the 67.62 s signal unambiguously as the white dwarf spin. Our photometric data shows that the ZZ Ceti pulsations detected near 5 min are extremely complex, with the dominant frequencies varying oil time scales of hours. We suggest that the complex pulsation pattern is related to the extremely rapid rotation of the white dwarf.

Item Type: Conference Item (UNSPECIFIED)
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science > Physics
Series Name: ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES
Journal or Publication Title: 15TH EUROPEAN WORKSHOP ON WHITE DWARFS, PROCEEDINGS
Publisher: ASTRONOMICAL SOC PACIFIC
ISBN: 978-1-58381-239-6
Editor: Napiwotzki, R and Burleigh, MR
Date: 2007
Volume: 372
Number of Pages: 6
Page Range: pp. 597-602
Publication Status: Published
Title of Event: 15th European Workshop on White Dwarfs
Location of Event: Univ Leicester, Leicester, ENGLAND
Date(s) of Event: AUG 07-11, 2006
URI: http://wrap.warwick.ac.uk/id/eprint/30864

Data sourced from Thomson Reuters' Web of Knowledge

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