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We present time dependent modeling based on the accretion disk limit cycle model for a 90 d light curve of the short period SU UMa-type dwarf nova V344 Lyr taken by Kepler. The unprecedented precision and cadence (1 minute) far surpass that generally available for long term light curves. The data encompass a super outburst, preceded by three normal (i.e., short) outbursts and followed by two normal outbursts. The main decay of the super outburst is nearly perfectly exponential, decaying at a rate approx.12 d/mag, while the much more rapid decays of the normal outbursts exhibit a faster-than-exponential shape. We show that the standard limit cycle model can account for the light curve, without the need for either the thermal-tidal instability or enhanced mass transfer

  • Creator/s: NASA Technical Reports Server (NTRS
  • Date: 1/1/2010
  • Year: 2010
  • Book Topics/Themes: NASA Technical Reports Server (NTRS), ACCRETION DISKS, LIGHT CURVE, THERMAL INSTABILITY, TIME DEPENDENCE, MASS TRANSFER, LYRA CONSTELLATION, DWARF NOVAE, TIDES, SHAPES, CATACLYSMIC VARIABLES, Cannizzo, J. K., Still, M. D., Howell, S. B., Wood, M. A., Smale, A. P

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