220 citations · 1.3k across the 46 of their papers we have counts for
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Mixing in classical novae: a 2-D sensitivity study
Jordi Casanova, Jordi Jose, Enrique Garcia-Berro +2
Classical novae are explosive phenomena that take place in stellar binary systems. They are powered by mass transfer from a low-mass, main sequence star onto a white dwarf. The mat…
Evaluating Systematic Dependencies of Type Ia Supernovae
Alan C. Calder, Brendan K. Krueger, Aaron P. Jackson +4
Type Ia supernovae are bright stellar explosions thought to occur when a thermonuclear runaway consumes roughly a solar mass of degenerate stellar material. These events produce an…
Evaluating Systematic Dependencies of Type Ia Supernovae: The Influence of Deflagration to Detonation Density
Aaron P. Jackson, Alan C. Calder, Dean M. Townsley +3
We explore the effects of the deflagration to detonation transition (DDT) density on the production of Ni-56 in thermonuclear supernova explosions (type Ia supernovae). Within the…
On variations of the brightness of type Ia supernovae with the age of the host stellar population
Brendan K. Krueger, Aaron P. Jackson, Dean M. Townsley +3
Recent observational studies of type Ia supernovae (SNeIa) suggest correlations between the peak brightness of an event and the age of the progenitor stellar population. This trend…
On mixing at the core-envelope interface during classical nova outbursts
Jordi Casanova, Jordi Jose, Enrique Garcia-Berro +2
Classical novae are powered by thermonuclear runaways that occur on the white dwarf component of close binary systems. During these violent stellar events, whose energy release is…