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20042009
most citedNewly Discovered Cataclysmic Variables from the INT/WFC Photometric H alpha Survey of the Northern Galactic Plane

39 citations · 124 across the 8 of their papers we have counts for

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astro-ph200834 cited

SDSS J080449.49+161624.8: A peculiar AM CVn star from a colour-selected sample of candidates

G. H. A. Roelofs, P. J. Groot, D. Steeghs +6

We describe a spectroscopic survey designed to uncover an estimated ~40 AM CVn stars hiding in the photometric database of the Sloan Digital Sky Survey (SDSS). We have constructed…

astro-ph200827 cited

ULTRACAM observations of two accreting white dwarf pulsators

C. M. Copperwheat, T. R. Marsh, V. S. Dhillon +6

In this paper we present high time-resolution observations of GW Librae and SDSS J161033.64-010223.3 -- two cataclysmic variables which have shown periodic variations attributed to…

astro-ph20089 cited

The hidden HI-massive LIRG HIZOA J0836-43: Inside-out galaxy formation

M. E. Cluver, T. H. Jarrett, P. N. Appleton +6

HIZOA J0836-43 is an extreme gas-rich (=7.5$\times10^{10} M_{\sun}$) disk galaxy which lies hidden behind the strongly obscuring Vela region of the Milky Way. Utilizin…

astro-ph200739 cited

Newly Discovered Cataclysmic Variables from the INT/WFC Photometric H alpha Survey of the Northern Galactic Plane

A. R. Witham, C. Knigge, A. Aungwerojwit +7

We report the discovery of 11 new cataclysmic variable (CV) candidates by the Isaac Newton Telescope (INT) Photometric H alpha Survey of the northern Galactic plane (IPHAS). Three…

astro-ph20078 cited

Outbursts of EX Hydrae Revisited

N. Mhlahlo, D. A. H. Buckley, V. Dhillon +3

We present optical spectroscopy of EX Hya during its 1991 outburst. This outburst is characterised by strong irradiation of the front face of the secondary star by the white dwarf,…

astro-ph20077 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.…