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Physical Sciences and Mathematics Commons

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Astrophysics and Astronomy

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Aerospace, Physics, and Space Science Faculty Publications

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2010

Novae

Articles 1 - 2 of 2

Full-Text Articles in Physical Sciences and Mathematics

The Kepler Light Curve Of V344 Lyrae: Constraining The Thermal-Viscous Limit Cycle Instability, John K. Cannizzo, Martin D. Still, Steve B. Howell, Matt A. Wood, Alan P. Smale Dec 2010

The Kepler Light Curve Of V344 Lyrae: Constraining The Thermal-Viscous Limit Cycle Instability, John K. Cannizzo, Martin D. Still, Steve B. Howell, Matt A. Wood, Alan P. Smale

Aerospace, Physics, and Space Science Faculty Publications

We present time-dependent modeling based on the accretion disk limit cycle model for a 270 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 two superoutbursts and 17 normal (i.e., short) outbursts. The main decay of the superoutbursts is nearly perfectly exponential, decaying at a rate ~12 d mag−1, while the much more rapid decays of the normal outbursts exhibit a faster-than-exponential shape. Our modeling using the basic accretion disk limit cycle can produce the …


Quiescent Superhumps Detected In The Dwarf Nova V344 Lyrae By Kepler, Martin D. Still, Steve B. Howell, Matt A. Wood, John K. Cannizzo, Alan P. Smale Jul 2010

Quiescent Superhumps Detected In The Dwarf Nova V344 Lyrae By Kepler, Martin D. Still, Steve B. Howell, Matt A. Wood, John K. Cannizzo, Alan P. Smale

Aerospace, Physics, and Space Science Faculty Publications

The timing capabilities and sensitivity of Kepler, NASA's observatory to find Earth-sized planets within the habitable zone of stars, are well matched to the timescales and amplitudes of accretion disk variability in cataclysmic variables. This instrumental combination provides an unprecedented opportunity to test and refine stellar accretion paradigms with high-precision, uniform data, and containing none of the diurnal or season gaps that limit ground-based observations. We present a 3 month, 1 minute cadence Kepler light curve of V344 Lyr, a faint, little-studied dwarf nova within the Kepler field. The light curve samples V344 Lyr during five full normal outbursts and …