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A high-mass X-ray binary descended from an ultra-stripped supernova
Noel D. Richardson, Clarissa Pavao, Jan J. Eldridge +6
Ultra-stripped supernovae are different from other terminal explosions of massive stars, as they show little or no ejecta from the actual supernova event. They are thought to occur…
The relationship between gamma Cassiopeiae's X-ray emission and its circumstellar environment
M. A. Smith, R. Lopes de Oliveira, C. Motch +17
γCas is the prototypical classical Be star and is best known for its variable hard X-ray emission. To elucidate the reasons for this emission, we mounted a multiwavelength campaign…
H-alpha Emission Variability in the gamma-ray Binary LS I +61 303
M. Virginia McSwain, Erika D. Grundstrom, Douglas R. Gies +1
LS I +61 303 is an exceptionally rare example of a high mass X-ray binary (HMXB) that also exhibits MeV-TeV emission, making it one of only a handful of "gamma-ray binaries". Here…