2006
DOI: 10.1111/j.1365-2966.2006.10788.x
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SDSS J160043.6+074802.9: a very rapid sdO pulsator

Abstract: We report the serendipitous discovery of the Sloan Digital Sky Survey star, SDSS J160043.6+074802.9 to be a very rapid pulsator. The variation is dominated by a frequency near 8380 microHz (period = 119.33 s) with a large amplitude (0.04 mag) and its first harmonic at 16760 microHz (59.66 s; 0.005 mag). In between these frequencies, we find at least another 8 variations with periods between 62 and 118 seconds and amplitudes between about 0.007 and 0.003 mag; weaker oscillations might also be present. Prelimina… Show more

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Cited by 65 publications
(68 citation statements)
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References 18 publications
(14 reference statements)
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“…, and has periods more typical for the V1093 Her stars than the V361 Hya stars which surrounds it in the T eff /log g plane. Furthermore, one single sdO has been recently discovered to be a very rapid multimode pulsator (Woudt et al 2006). Observational searches for more sdO pulsators are ongoing, but evidence so far indicates that pulsations among these stars are rare (Rodríguez-López et al 2007).…”
Section: Introductionmentioning
confidence: 99%
“…, and has periods more typical for the V1093 Her stars than the V361 Hya stars which surrounds it in the T eff /log g plane. Furthermore, one single sdO has been recently discovered to be a very rapid multimode pulsator (Woudt et al 2006). Observational searches for more sdO pulsators are ongoing, but evidence so far indicates that pulsations among these stars are rare (Rodríguez-López et al 2007).…”
Section: Introductionmentioning
confidence: 99%
“…For completeness, although these objects will not be discussed further in this short paper, we have to mention that hot subdwarfs also host pulsators in the very high temperature range where sdO stars are found (Figure 1). The first pulsating star of this type was discovered by Woudt et al (2006) and shows very rapid oscillations (P ∼ 40 − 150 s) associated with low-order p-modes. Surprisingly, this star remains so far the unique member of this class found among the field sdO stars, despite significant efforts to search for pulsations in such objects (Rodríguez-López et al 2008).…”
Section: Pulsations In Hot Subdwarfsmentioning
confidence: 99%
“…The second group, discovered by (Green et al 2003) and called V1093 Her stars, exhibits periods from 45 min to a few hours (Van Grootel et al 2013b). The first He-sdBV pulsator was VARIABLE STARS 423 discovered by Ahmad & Jeffery (2005) and the first sdOV by Woudt et al (2006). The Kepler satellite has had a transformational impact on the asteroseismology of V1093 Her stars, providing rotation diagnostics and, with time variable multiplet spacings, challenging conventional models of sdB interiors (e.g.…”
Section: Compact Oscillatorsmentioning
confidence: 99%