75 citations · 121 across the 4 of their papers we have counts for
5 papers
SU Lyn: diagnosing the boundary layer with UV and hard X-ray data
Raimundo Lopes de Oliveira, Jennifer Sokoloski, Gerardo Juan Luna +2
Symbiotic stars in which the symbiotic phenomenon is powered solely by accretion, often at an average rate that is higher than in cataclysmic variable stars, provide an important o…
The X-ray Evolution of the Symbiotic Star V407 Cygni during its 2010 Outburst
Koji Mukai, Thomas Nelson, Laura Chomiuk +2
We present a summary of Swift and Suzaku X-ray observations of the 2010 nova outburst of the symbiotic star, V407 Cyg. The Suzaku spectrum obtained on day 30 indicates the presence…
The Fall and the Rise of X-rays from Dwarf Novae in Outburst: RXTE Observations of VW Hydri and WW Ceti
Derek Fertig, Koji Mukai, Thomas Nelson +1
In a dwarf nova, the accretion disk around the white dwarf is a source of ultraviolet, optical, and infrared photons, but is never hot enough to emit X-rays. Observed X-rays instea…
Analysis of a State Changing Supersoft X-ray Source in M31
Brandon Patel, Rosanne Di Stefano, Thomas Nelson +3
We report on observations of a luminous supersoft X-ray source (SSS) in M31, r1-25, that has exhibited spectral changes to harder X-ray states. We document these spectral changes.…
NLTE model atmospheres for the hottest white dwarfs: Spectral analysis of the compact component in nova V4743 Sgr
T. Rauch, M. Orio, R. Gonzales-Riestra +4
Half a year after its outburst in September 2002, nova V4743 Sgr evolved into the brightest supersoft X-ray source in the sky with a flux maximum around 30A. We calculated grids of…