126 citations · 1.3k across the 37 of their papers we have counts for
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Dissecting a disk-instability outburst in a symbiotic star: , and observations of T Coronae Borealis during the rise to the "super-active" state
G. J. M. Luna, T. Nelson, K. Mukai +1
The current state of the recurrent nova T CrB has been observed with unprecedented detail. Previously published observations provide strong evidence that this state…
X-ray, UV, and optical observations of the accretion disk and boundary layer in the symbiotic star RT Cru
G. J. M. Luna, K. Mukai, J. L. Sokoloski +8
Compared to mass transfer in cataclysmic variables, the nature of accretion in symbiotic binaries in which red giants transfer material to white dwarfs (WDs) has been difficult to…
A Detailed Observational Analysis of V1324 Sco, the Most Gamma-Ray Luminous Classical Nova to Date
Thomas Finzell, Laura Chomiuk, Brian D. Metzger +32
It has recently been discovered that some, if not all, classical novae emit GeV gamma rays during outburst, but the mechanisms involved in the production of the gamma rays are stil…
SU Lyncis, a hard X-ray bright M giant: Clues point to a large hidden population of symbiotic stars
K. Mukai, G. J. M. Luna, G. Cusumano +6
Symbiotic star surveys have traditionally relied almost exclusively on low resolution optical spectroscopy. However, we can obtain a more reliable estimate of their total Galactic…
Shock-powered radio emission from V5589 Sagittarii (Nova Sgr 2012 1)
Jennifer H. S. Weston, J. L. Sokoloski, Laura Chomiuk +7
Since the Fermi discovery of -rays from novae, one of the biggest questions in the field has been how novae generate such high-energy emission. Shocks must be a fundamental ingr…
Swift detection of the super-swift switch-on of the super-soft phase in nova V745 Sco (2014)
K. L. Page, J. P. Osborne, N. P. M. Kuin +15
V745 Sco is a recurrent nova, with the most recent eruption occurring in February 2014. V745 Sco was first observed by Swift a mere 3.7 hr after the announcement of the optical dis…