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Filtering by: Identifier tesim 0004-637X Remove constraint Identifier tesim: 0004-637X

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  • Qv33rx953?file=thumbnail
    Article
    Mukai, Koji
    We present optical and X-ray time series photometry of EI UMa that reveal modulation at 746 and 770 s, which we interpret as the white dwarf spin and spin-orbit sidebands. These detections, combined with previous X-ray studies, establish EI UMa as an . . .
  • Nk322f49w?file=thumbnail
    Article
    Shankland, P. D.
    We report the results of a globally coordinated photometric campaign to search for transits by the P ~ 30 day and P ~ 60 day outer planets of the three-planet system orbiting the nearby M dwarf Gl 876. These two planets experience strong mutual pertur . . .
  • W3763838r?file=thumbnail
    Article
    Mukai, K.
    DQ Herculis (Nova Herculis 1934) is a deeply eclipsing cataclysmic variable containing a magnetic white dwarf primary.The accretion disk is thought to block our line of sight to the white dwarf at all orbital phases due to its extreme inclination angl . . .
  • 9s161776s?file=thumbnail
    Article
    Mukai, K.
    DQ Herculis (Nova Herculis 1934) is a deeply eclipsing cataclysmic variable containing a magnetic white dwarf primary. The accretion disk is thought to block our line of sight to the white dwarf at all orbital phases because of its extreme inclination . . .