activity
19952011
most citedULTRACAM: an ultra-fast, triple-beam CCD camera for high-speed astrophysics

343 citations · 1.7k across the 45 of their papers we have counts for

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Showing 2004 · astro-phShow all

11 papers · 2 filters

astro-ph2004

Geometrical constraints upon the unipolar model of V407 Vul and RXJ0806.3+1527

S. C. C. Barros, T. R. Marsh, P. Groot +5

V407 Vul and RX J0806.3+1527 are X-ray emitting stars with X-ray light curves that are 100% modulated on periods of 569 and 321 seconds respectively. These periods and no others ar…

astro-ph2004

Rotational period of WD1953-011 - a magnetic white dwarf with a star spot

C. S. Brinkworth, T. R. Marsh, L. Morales-Rueda +3

WD1953-011 is an isolated, cool (7920 +/- 200K, Bergeron, Legget & Ruiz, 2001) magnetic white dwarf (MWD) with a low average field strength (~70kG, Maxted et al. 2000) and a higher…

astro-ph2004

Multi-epoch Spectroscopy of IY UMa: Quiescence, Rise, Normal Outburst & Superoutburst

Daniel J. Rolfe, Carole A. Haswell, Timothy M. C. Abbott +3

We exploit rare observations covering the time before and during a normal outburst in the deeply-eclipsing SU UMa system IY UMa to study the dramatic changes in the accretion flow…

astro-ph20043 cited

Subdwarf B Binaries from the Edinburgh--Cape Survey

L. Morales-Rueda, P. F. L. Maxted, T. R. Marsh +2

We present the first results of a campaign to obtain orbital solutions of subdwarf B (sdB) stars from the Edinburgh-Cape survey. We have obtained blue spectra of 35 sdBs, 20 of whi…

astro-ph2004

HS2331+3905: The cataclysmic variable that has it all

S. Araujo-Betancor, B. T. Gaensicke, H. -J. Hagen +6

We report detailed follow-up observations of the cataclysmic variable HS2331+3905, identified as an emission-line object in the Hamburg Quasar Survey. An orbital period of 81.08min…

astro-ph2004

Detection of the white dwarf and the secondary star in the new SU UMa dwarf nova HS 2219+1824

P. Rodriguez-Gil, B. T. Gaensicke, H. -J. Hagen +4

We report the discovery of a new, non-eclipsing SU UMa-type dwarf nova, HS 2219+1824. Photometry obtained in quiescence (V ~ 17.5) reveals a double-humped light curve from which we…