59 citations · 273 across the 15 of their papers we have counts for
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Evolution of the recent high-accretion state of the recurrent nova T CrB: HST, Swift, NuSTAR, and XMM-Newton observations
G. J. M. Luna, N. P. M. Kuin, K. Mukai +3
As the recurrent nova T Coronae Borealis (T CrB) approaches its next predicted thermonuclear eruption, it is currently exhibiting a "super-active state" (SAS) characterized by enha…
Swift observations of the 2015 outburst of AG Peg -- from slow nova to classical symbiotic outburst
Gavin Ramsay, J. L. Sokoloski, G. J. M. Luna +1
Symbiotic stars often contain white dwarfs with quasi-steady shell burning on their surfaces. However, in most symbiotics, the origin of this burning is unclear. In symbiotic slow…
Testing the cooling flow model in the intermediate polar EX Hydrae
G. J. M. Luna, J. C. Raymond, N. S. Brickhouse +3
We use the best available X-ray data from the intermediate polar EX Hydrae to study the cooling-flow model often applied to interpret the X-ray spectra of these accreting magnetic…
Chandra detection of extended X-ray emission from the recurrent nova RS Ophiuchi
G. J. M. Luna, R. Montez, J. L. Sokoloski +2
Radio, infrared, and optical observations of the 2006 eruption of the symbiotic recurrent nova RS Ophiuchi (RS Oph) showed that the explosion produced non-spherical ejecta. Some of…