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20022020
most citedSuperhumps in Cataclysmic Binaries. XXV. q_crit, epsilon(q), and Mass-Radius

239 citations · 736 across the 17 of their papers we have counts for

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astro-ph2007★ 7 cited

The Discovery of a Persistent Quasi-Periodic Oscillation in the Intermediate Polar TX Col

N. Mhlahlo, D. A. H. Buckley, V. S. Dhillon +8

We report on the detection of an ~5900 s quasi-periodic variation in the extensive photometry of TX Col spanning 12 years. We discuss five different models to explain this period.…

astro-ph2005★ 239 cited

Superhumps in Cataclysmic Binaries. XXV. q_crit, epsilon(q), and Mass-Radius

Joseph Patterson, Jonathan Kemp, David Harvey +17

We report on successes and failures in searching for positive superhumps in cataclysmic variables, and show the superhumping fraction as a function of orbital period. Basically, al…

astro-ph2003★ 85 cited

Superhumps in Cataclysmic Binaries. XXIV. Twenty More Dwarf Novae

J. Patterson, J. Thorstensen, J. Kemp +23

We report precise measures of the orbital and superhump period in twenty more dwarf novae. For ten stars, we report new and confirmed spectroscopic periods - signifying the orbital…

astro-ph2002★ 69 cited

Superhumps in Cataclysmic Binaries. XXIII. V442 Ophiuchi and RX J1643.7+3402

Joseph Patterson, William Fenton, John Thorstensen +15

We report the results of long observing campaigns on two novalike variables: V442 Ophiuchi and RX J1643.7+3402. These stars have high-excitation spectra, complex line profiles sign…

astro-ph2002★ 149 cited

The 2001 Superoutburst of WZ Sagittae

J. Patterson, G. Masi, M. Richmond +25

We report the results of a worldwide campaign to observe WZ Sagittae during its 2001 superoutburst. After a 23-year slumber at V=15.5, the star rose within 2 days to a peak brightn…

astro-ph2002★ 23 cited

Superhumps in Cataclysmic Binaries. XXII. 1RXS J232953.9+062814

David Skillman, Thomas Krajci, Edward Beshore +7

We report photometry of 1RXS J232953.9+062814, a recently discovered dwarf nova with a remarkably short 64.2-minute orbital period. In quiescence, the star's light curve is that of…