37 citations · 56 across the 4 of their papers we have counts for
5 papers
On the Nature of the BeWD System Nova FQ Circinus
Shatakshi Chamoli, Philip A. Charles, Judhajeet Basu +3
The classical nova FQ Cir (Schaefer et al. 2026) has recently been shown to have a Be star donor, and has been identified as a High Mass Cataclysmic Variable (HMCV), with an orbita…
Discovering Cataclysmic Variables from the Rubin Observatory LSST
D. A. H. Buckley, Y. Tampo, P. Szkody +8
The Vera C. Rubin Observatory's Legacy Survey of Space and Time (LSST) will provide a windfall of new transients and variable sources. Here we have performed mock observation simul…
Triggering micronovae through magnetically confined accretion flows in accreting white dwarfs
S. Scaringi, P. J. Groot, C. Knigge +5
Rapid bursts at optical wavelengths have been reported for several accreting white dwarfs, where the optical luminosity can increase by up to a factor 30 in less than an hour fadin…
Localised thermonuclear bursts from accreting magnetic white dwarfs
S. Scaringi, P. J. Groot, C. Knigge +16
Nova explosions are caused by global thermonuclear runaways triggered in the surface layers of accreting white dwarfs. It has been predicted that localised thermonuclear bursts on…
An accreting white dwarf displaying fast transitional mode switching
S. Scaringi, D. de Martino, D. H. Buckley +6
Accreting white dwarfs are often found in close binary systems with orbital periods ranging from tens of minutes to several hours. In most cases, the accretion process is relativel…