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SDSS J160043.6+074802.9: a very rapid sdO pulsator
P. A. Woudt 1★ , D. Kilkenny 2 , E. Zietsman 3 , B. Warner 1 , N. S. Loaring 2 , C. Copley 3 , A. Kniazev 2 , P. Väisänen 2 , M. Still 2 , R. S. Stobie 2 , E. B. Burgh 4 , K. H. Nordsieck 4 , J. W. Percival 4 , D. O'Donoghue 2 and D. A. H. Buckley 2
  1 Department of Astronomy, University of Cape Town, Private Bag X3, Rondebosch 7701, South Africa   2 South African Astronomical Observatory, PO Box 9, Observatory 7935, South Africa   3 National Astrophysics and Space Science Programme, University of Cape Town, Rondebosch 7700, South Africa   4 Space Astronomy Laboratory, University of Wisconsin, Madison, WI 53706, USA
Correspondence to   E-mail: pwoudt@circinus.ast.uct.ac.za
Copyright 2006 The Authors. Journal compilation © 2006 RAS
KEYWORDS
stars: individual: SDSS J160043.6+074802.9 • stars: oscillations • stars: variables: other.

ABSTRACT

We report the serendipitous discovery of the Sloan Digital Sky Survey (SDSS) star SDSS J160043.6+074802.9 to be a very rapid pulsator. The variation is dominated by a frequency near 8380 μHz (period = 119.33 s) with a large amplitude (0.04 mag) and its first harmonic at 16760 μHz (59.66 s; 0.005 mag). In between these frequencies, we find at least another eight variations with periods between 62 and 118 s and amplitudes between about 0.007 and 0.003 mag; weaker oscillations might also be present. Preliminary spectrograms from the performance verification phase of the Southern African Large Telescope indicate that SDSS J160043.6+074802.9 is a spectroscopic binary consisting of an sdO star and a late-type main-sequence companion. This makes it the first unambiguous detection of such an sdO star to pulsate, and certainly the first found to exhibit multifrequency variations.


Accepted 2006 July 8. Received 2006 July 7; in original form 2006 May 22

DIGITAL OBJECT IDENTIFIER (DOI)
10.1111/j.1365-2966.2006.10788.x About DOI

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