activity
19972022
most citedCombining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes

127 citations · 2.2k across the 71 of their papers we have counts for

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Showing 2002 · astro-phShow all

8 papers · 2 filters

astro-ph2002★ 13 cited

RX J1039.7-0507: A New Intermediate Polar and Probable Recent Nova, possessing a large Reflection Effect

Patrick A. Woudt, Brian Warner

The ROSAT source RX J1039.7-0507, known from its optical spectrum to be a Cataclysmic Variable star, is shown from high speed photometry to have an orbital period of 1.574 h. The s…

astro-ph2002★ 13 cited

Nova Scorpii 1941 (V697 Sco): A Probable Intermediate Polar

Brian Warner, Patrick A. Woudt

V697 Sco, the remnant of Nova Scorpii 1941 and currently at V ~ 20.0, is found from photometric observations to have the characteristics of an intermediate polar (IP) with an orbit…

astro-ph2002

The UCT Survey of Old Novae

Patrick A. Woudt, Brian Warner

We present a status report on our high speed photometric survey of faint Cataclysmic Variables, which is concentrating on old novae.

astro-ph2002★ 12 cited

General Properties of Quiescent Novae

Brian Warner

The observed properties of novae before and after eruption are discussed. The distribution of orbital periods of novae shows a concentration near 3.2 h, which resembles that of mag…

astro-ph2002★ 92 cited

Dwarf Nova Oscillations and Quasi-Periodic Oscillations in Cataclysmic Variables: II. A Low Inertia Magnetic Accretor Model

Brian Warner, Patrick A. Woudt

The Dwarf Nova Oscillations observed in Cataclysmic Variable (CV) stars are interpreted in the context of a Low Inertia Accretor model, in which accretion on to an equatorial belt…

astro-ph2002★ 49 cited

High speed photometry of faint Cataclysmic Variables: II. RS Car, V365 Car,] V436 Car, AP Cru, RR Cha, BI Ori, CM Phe and V522 Sgr

Patrick A. Woudt, Brian Warner

Short time scale photometric properties of eight faint Cataclysmic Variable (CV) stars are presented. Nova Carinae 1895 (RS Car) has a photometric modulation at 1.977 h which could…