22 citations · 22 across the 3 of their papers we have counts for
4 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…
eRASSU J043115.8-711730 :the first pulsating symbiotic super-soft X-ray source in the Magellanic Bridge
Tathagata Saha, Chandreyee Maitra, Philip Charles +9
The Magellanic Bridge stellar population is a relic of the tidal interaction between the Large and Small Magellanic Clouds. A comprehensive view of the evolution of the Bridge stel…
[HP99] 159 -- Properties of the first Supersoft X-ray Source with a Helium star donor
Hélène Szegedi, Philip A. Charles, David A. H. Buckley +3
[HP99] 159 is remarkable as the first supersoft X-ray source (SSS) identified with an evolved helium star donor. With a likely orbital period of 1.164 d or 2.327 d, the origin of t…
Orbital and Superorbital Monitoring of the Be/X-ray binary A0538-66: constraints on the system parameters
A. F. Rajoelimanana, P. A. Charles, P. J. Meintjes +3
We combine the decade long photometry of the Be/X-ray binary system A0538-66 provided by the MACHO and OGLE IV projects with high resolution SALT spectroscopy to provide detailed c…