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Results 1 - 5 of 5

Three-dimensional simulations of the interaction between the nova ejecta, the accretion disk, and the companion star. (arXiv:1712.08402v1 [astro-ph.SR])
- Virtual Journal - Volume 15, Issue 52 - article #8
- Joana Figueira (UPC Barcelona), Jordi Jose (UPC Barcelona), Enrique Garcia-Berro (UPC Barcelona), Simon W. Campbell (MPI Astrophysics Garching, Monash U), Domingo Garcia-Senz (UPC Barcelona), Shazrene Mohamed (SAAP Cape Town)
- http://arxiv.org/abs/1712.08402
Pulsating reverse detonation models of Type Ia supernovae. I: Detonation ignition
- Virtual Journal - Volume 7, Issue 4 - article #7
- Eduardo Bravo, Domingo Garcia-Senz
- arXiv.org - Astrophysics - Volume: 2009, Issue: 22 Jan
- arXiv:0901.3008 [ps, pdf, other]
Pulsating reverse detonation models of Type Ia supernovae. II: Explosion
- Virtual Journal - Volume 7, Issue 4 - article #8
- Eduardo Bravo, Domingo Garcia-Senz, Ruben M. Cabezon, Inmaculada Dominguez
- arXiv.org - Astrophysics - Volume: 2009, Issue: 22 Jan
- arXiv:0901.3013 [ps, pdf, other]
Beyond the bubble catastrophe of Type Ia supernovae: Pulsating Reverse Detonation models
- Virtual Journal - Volume 4, Issue 14 - article #8
- Eduardo Bravo, Domingo Garcia-Senz
- ArXiv - Astrophysics
- astro-ph/0604025 [abs, ps, pdf, other]
Explosion models for thermonuclear supernovae resulting from different ignition conditions
- Virtual Journal - Volume 2, Issue 2 - article #16
- Eduardo Bravo, Domingo Garcia-Senz
- arXiv.org – Astrophysics – January 2004
- astro-ph/0401230 [ abs , ps , pdf , other ]

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