activity
20012008
most citedThe mass of the white dwarf in the recurrent nova U Scorpii

102 citations · 201 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph2008★ 26 cited

GD 552: a cataclysmic variable with a brown dwarf companion?

E. Unda-Sanzana, T. R. Marsh, B. T. Gansicke +7

GD 552 is a high proper motion star with the strong, double-peaked emission lines characteristic of the dwarf nova class of cataclysmic variable star, and yet no outburst has been…

astro-ph2004★ 34 cited

The component masses of the cataclysmic variable V347 Puppis

T. D. Thoroughgood, V. S. Dhillon, D. Steeghs +7

We present time-resolved spectroscopy and photometry of the double-lined eclipsing cataclysmic variable V347 Pup (= LB 1800). There is evidence of irradiation on the inner hemisphe…

astro-ph2004★ 39 cited

The masses of the cataclysmic variables AC Cancri and V363 Aurigae

T. D. Thoroughgood, V. S. Dhillon, C. A. Watson +3

We present time-resolved spectroscopy and photometry of the double-lined eclipsing cataclysmic variables AC Cnc and V363 Aur (= Lanning 10). There is evidence of irradiation on the…

astro-ph2001

The Recurrent Nova U Scorpii - A Type Ia Supernova Progenitor

T. D. Thoroughgood, V. S. Dhillon, S. P. Littlefair +2

We derive the mass of the white dwarf in the eclipsing recurrent nova U Sco from the radial velocity semi-amplitudes of the primary and secondary stars. Our results give a high whi…

astro-ph2001★ 102 cited

The mass of the white dwarf in the recurrent nova U Scorpii

T. D. Thoroughgood, V. S. Dhillon, S. P. Littlefair +2

We present spectroscopy of the eclipsing recurrent nova U Sco. The radial velocity semi-amplitude of the primary star was found to be K_W = 93 \pm 10 kms^{-1} from the motion of th…