MESA inlists associated with He-accreting carbon-oxygen white dwarfs and Type Ia supernova
Accreting white dwarfs can exhibit a variety of thermonuclear phenomena, such as shell flashes, clas...
Sub-Chandrasekhar mass carbon-oxygen white dwarfs with a surface helium shell have been proposed as ...
Context. The study of Type Ia supernovae (SNIa) has lead to greatly improved insights into...
He accretion onto carbon-oxygen white dwarfs (CO WDs) plays a fundamental role when studying the for...
Abstract: Type Ia supernovae are thought to result from thermonuclear explosions of carbon-oxygen wh...
MESA inlist associated files for The outcomes of carbon-oxygen white dwarfs accreting CO-rich materi...
Employing the MESA stellar evolution code, we computed He accretion onto carbon-oxygen white dwarfs ...
The final fate of accreting C + O white dwarfs is either thermonuclear explosion or collapse, if the...
10 pages, 2 tables.-- En: "Supernovae: lights in the darkness", October 3-5, 2007, Mao (Menorca), t...
Recent studies have argued that the progenitor system of type Iax supernovae must consist of a carbo...
Supernovae are some of the brightest and most energetic explosions in the universe. In the mid- to l...
Recent extensive observations of Type Ia Supernovae (SNe Ia) have revealed the existence of a divers...
While it is generally agreed that type Ia supernovae are thermonuclear explosions of carbon-oxygen w...
I argue that the observational evidence for white dwarf-white dwarf mergers supports the view that t...
Over the past few years, we have been investigating the effects of accretion onto massive white dwar...
Accreting white dwarfs can exhibit a variety of thermonuclear phenomena, such as shell flashes, clas...
Sub-Chandrasekhar mass carbon-oxygen white dwarfs with a surface helium shell have been proposed as ...
Context. The study of Type Ia supernovae (SNIa) has lead to greatly improved insights into...
He accretion onto carbon-oxygen white dwarfs (CO WDs) plays a fundamental role when studying the for...
Abstract: Type Ia supernovae are thought to result from thermonuclear explosions of carbon-oxygen wh...
MESA inlist associated files for The outcomes of carbon-oxygen white dwarfs accreting CO-rich materi...
Employing the MESA stellar evolution code, we computed He accretion onto carbon-oxygen white dwarfs ...
The final fate of accreting C + O white dwarfs is either thermonuclear explosion or collapse, if the...
10 pages, 2 tables.-- En: "Supernovae: lights in the darkness", October 3-5, 2007, Mao (Menorca), t...
Recent studies have argued that the progenitor system of type Iax supernovae must consist of a carbo...
Supernovae are some of the brightest and most energetic explosions in the universe. In the mid- to l...
Recent extensive observations of Type Ia Supernovae (SNe Ia) have revealed the existence of a divers...
While it is generally agreed that type Ia supernovae are thermonuclear explosions of carbon-oxygen w...
I argue that the observational evidence for white dwarf-white dwarf mergers supports the view that t...
Over the past few years, we have been investigating the effects of accretion onto massive white dwar...
Accreting white dwarfs can exhibit a variety of thermonuclear phenomena, such as shell flashes, clas...
Sub-Chandrasekhar mass carbon-oxygen white dwarfs with a surface helium shell have been proposed as ...
Context. The study of Type Ia supernovae (SNIa) has lead to greatly improved insights into...