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Related papers: SDSS J160043.6+074802.9: a very rapid sdO pulsator

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A spectroscopic analysis of SDSS J160043.6+074802.9, a binary system containing a pulsating subdwarf-O (sdO) star with a late-type companion, yields Teff = 70 000 +/- 5000 K and log g = 5.25 +/- 0.30, together with a most likely type of K3V…

Solar and Stellar Astrophysics · Physics 2015-05-14 C. Rodríguez-López , A. E. Lynas-Gray , D. Kilkenny , J. MacDonald , A. Moya , C. Koen , P. A. Woudt , D. J. Wium , B. Oruru , E. Zietsman

The Sloan Digital Sky Survey (SDSS) source J102347.6+003841 was recently revealed to be a binary 1.69 millisecond radio pulsar with a 4.75 hr orbital period and a ~0.2 M_sun companion. Here we analyze the SDSS spectrum of the source in…

High Energy Astrophysical Phenomena · Physics 2009-09-24 Zhongxiang Wang , Anne M. Archibald , John R. Thorstensen , Victoria M. Kaspi , Duncan R. Lorimer , Ingrid Stairs , Scott M. Ransom

We present follow-up time-series photometric observations that confirm and extend the results of the significant discovery made by Barlow et al.(2008) that the Hot DQ white dwarfs SDSS J220029.08-074121.5 and SDSS J234843.30-094245.3 are…

Solar and Stellar Astrophysics · Physics 2015-05-13 P. Dufour , E. M. Green , G. Fontaine , P. Brassard , M. Francoeur , M. Latour

We find from high speed photometry of the Sloan Digital Survey cataclysmic variable candidate SDSS J161033.64-010223.3 that it has a double humped modulation, which is probably orbital, with a period of 80.52 minutes, and shows strong ZZ…

Astrophysics · Physics 2009-11-10 Patrick A. Woudt , Brian Warner

High speed photometric observations of the spectroscopically-discovered PG 1159 star SDSS J034917.41-005917.9 in 2007 and 2009 reveal a suite of pulsation frequencies in the range of 1038 - 3323 microHz with amplitudes between 3.5 and 18.6…

Solar and Stellar Astrophysics · Physics 2015-06-11 Patrick A. Woudt , Brian Warner , Ewald Zietsman

We report the discovery of two new accreting pulsating white dwarf stars amongst the cataclysmic variables of the Sloan Digital Sky Survey: SDSSJ074531.91+453829.5 and SDSSJ091945.10+085710.0. We observe high amplitude non-sinusoidal…

We have obtained time-series spectra for the pulsating hot subdwarf (sdB) PG1605+072. Previous time-series photometry of this star has shown maximum amplitude variations of about 0.1 mag and at least 50 periods. The pulsator has the largest…

Astrophysics · Physics 2007-05-23 Simon J. O'Toole , Teresa C. Teixeira , Timothy R. Bedding , Hans Kjeldsen

We searched the SuperWASP archive for objects displaying multiply periodic photometric variations. Specifically we sought evidence for eclipsing binary stars displaying a further non-harmonically related signal in their power spectra. The…

Solar and Stellar Astrophysics · Physics 2016-02-17 A. J. Norton , M. E. Lohr , B. Smalley , P. J. Wheatley , R. G. West

SDSSJ125733.63+542850.5 (hereafter SDSSJ1257+5428) is a compact white dwarf binary from the Sloan Digital Sky Survey that exhibits high-amplitude radial velocity variations on a period of 4.56 hours. While an initial analysis suggested the…

Solar and Stellar Astrophysics · Physics 2015-05-18 T. R. Marsh , B. T. Gaensicke , D. Steeghs , J. Southworth , D. Koester , V. Harris , L. Merry

SDSS J111215.82+111745.0 is the second pulsating extremely low-mass white dwarf discovered. Two short-period pulsations, 107.56 and 134.275 s, were detected on this star, which would be the first observed pressure mode ($p$-mode) pulsations…

Solar and Stellar Astrophysics · Physics 2023-02-08 Jie Su , Yan Li

We present the results of photometric observations of SDSS J080434.20+510349.2 in its low state and during an outburst and spectroscopy during the outburst. We found such peculiarities as a long-term outburst with amplitude probably not…

Photometric and spectroscopic observations reveal the Sloan Digital Sky Survey cataclysmic variable SDSS J132723.39+652854.2 to be a likely SW Sex star with an orbital period of P = 3.28 hours. The Sloan Digital Sky Survey spectrum shows…

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…

Astrophysics · Physics 2009-11-13 B. N. Barlow , B. H. Dunlap , R. Rosen , J. C. Clemens

We report the discovery of pulsations in the spectroscopic PG 1159 type pre-white dwarf SDSS J075415.12+085232.18. Analysis of the spectrum by Werner, Rauch and Kepler (2014) indicated Teff=120 000+/-10 000 K, log g=7.0+/-0.3, mass…

Solar and Stellar Astrophysics · Physics 2015-06-19 S. O. Kepler , Luciano Fraga , Don Earl Winget , Keaton Bell , Alejandro H. Corsico , Klaus Werner

We present the analysis of time-resolved spectroscopy of the pulsating sdB star PG1605+072. From our main observing run of 16 nights we have detected velocity variations at 5 frequencies that correspond to those found in photometry. Based…

Astrophysics · Physics 2009-11-07 S. J. O'Toole , T. R. Bedding , H. Kjeldsen , T. H. Dall , D. Stello

We describe a spectroscopic survey designed to uncover an estimated ~40 AM CVn stars hiding in the photometric database of the Sloan Digital Sky Survey (SDSS). We have constructed a relatively small sample of about 1500 candidates based on…

We report the discovery of SDSS J133725.26+395237.7 (hereafter SDSS J1337+3952), a double-lined white dwarf (WD+WD) binary identified in early data from the fifth generation Sloan Digital Sky Survey (SDSS-V). The double-lined nature of the…

We present high speed photometry of the Sloan Digital Sky Survey cataclysmic variable SDSS J013701.06-091234.9 in quiescence and during its 2003 December superoutburst. The orbital modulation at 79.71\pm0.01 min is double humped; the…

Astrophysics · Physics 2009-11-10 M. L. Pretorius , P. A. Woudt , B. Warner , G. Bolt , J. Patterson , E. Armstrong

We present the results of a search for pulsations in six of the recently discovered carbon-atmosphere white dwarf ("hot DQ") stars. Based on our theoretical calculations, the star SDSS J142625.71+575218.3 is the only object expected to…

We report on 22 yrs of radio timing observations of the millisecond pulsar J1024$-$0719 by the telescopes participating in the European Pulsar Timing Array (EPTA). These observations reveal a significant second derivative of the pulsar spin…

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