467 citations · 4.2k across the 127 of their papers we have counts for
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astro-ph.SR2026
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…
astro-ph.SR2021★ 19 cited
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…