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most citedSDSSJ104341.53+085558.2: A second white dwarf with a gaseous debris disc

129 citations · 359 across the 6 of their papers we have counts for

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10 papers

astro-ph.SR200937 cited

Post common envelope binaries from SDSS. IV: SDSSJ121258.25-012310.1, a new eclipsing system

A. Nebot Gómez-Morán, A. D. Schwope, M. R. Schreiber +8

From optical photometry we show that SDSSJ121258.25-012310.1 is a new eclipsing, post common-envelope binary with an orbital period of 8.06 hours and an eclipse length of 23 minute…

astro-ph200876 cited

Post Common Envelope Binaries from SDSS. V: Four eclipsing white dwarf main sequence binaries

S. Pyrzas, B. T. Gänsicke, T. R. Marsh +7

We identify SDSS011009.09+132616.1, SDSS030308.35+005444.1, SDSS143547.87+373338.5 and SDSS154846.00+405728.8 as four eclipsing white dwarf plus main sequence (WDMS) binaries from…

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-ph200850 cited

Post Common Envelope Binaries from SDSS - III. Seven new orbital periods

A. Rebassa-Mansergas, B. T. Gaensicke, M. R. Schreiber +11

We present follow-up spectroscopy and photometry of 11 post common envelope binary (PCEB) candidates identified from multiple Sloan Digital Sky Survey (SDSS) spectroscopy in an ear…

astro-ph200740 cited

Post common envelope binaries from SDSS. II: Identification of 9 close binaries with VLT/FORS2

M. R. Schreiber, B. T. Gaensicke, J. Southworth +2

The Sloan Digital Sky Survey turned out to be very efficient in identifying white dwarf/main sequence binaries (WDMS). The population of WDMS systems consists of wide systems whose…

astro-ph2007129 cited

SDSSJ104341.53+085558.2: A second white dwarf with a gaseous debris disc

B. T. Gaensicke, T. R. Marsh, J. Southworth

Intermediate resolution spectroscopy of the white dwarf SDSSJ104341.53+085558.2 contains double-peaked emission lines of CaII8498,8542,8662 and identifies this object to be the sec…