Add to ORKGSIGLEAvailable from: http://www.mpa-garching.mpg.de / FIZ - Fachinformationszzentrum Karlsruhe / TIB - Technische InformationsbibliothekDEGerman
SIGLEAvailable from: http://www.mpa-garching.mpg.de / FIZ - Fachinformationszzentrum Karlsruhe / TIB...
In order to deal with dynamical phenomena of stars, gasdynamical equations and, especially, the shoc...
We perform radiation hydrodynamic simulations to study how very massive stars recover from giant eru...
What happens at the end of the life of massive stars? At one time we thought all these stars followe...
Supernovae are grand and extraordinarily energetic explosions that signify the death of a star. Ther...
Shock-heating of stellar envelopes: A possible common mechanism at the origin of explosions and eru...
How a massive star ends its life depends upon how that life has been lived - the rotation, mass and ...
Explosive astrophysical phenomena have historically played a significant role in understanding the u...
SIGLECopy held by FIZ Karlsruhe; available from UB/TIB Hannover / FIZ - Fachinformationszzentrum Kar...
The impact of rapid rotation of the supernova progenitor star (white dwarf) on its explosion (type I...
Open AccessGamma ray bursts which are first detected in energetic gamma rays and which then glow in ...
SIGLEAvailable from: http://www.mpa-garching.mpg.de / FIZ - Fachinformationszzentrum Karlsruhe / TIB...
Binary star systems known as cataclysmic variables can exhibit violent explosions called novae. Obse...
SIGLEAvailable from: http://www.mpa-garching.mpg.de / FIZ - Fachinformationszzentrum Karlsruhe / TIB...
Durant les dix dernières années, les développements du logiciel d'évolution stellaire de Genève ont ...
SIGLEAvailable from: http://www.mpa-garching.mpg.de / FIZ - Fachinformationszzentrum Karlsruhe / TIB...
In order to deal with dynamical phenomena of stars, gasdynamical equations and, especially, the shoc...
We perform radiation hydrodynamic simulations to study how very massive stars recover from giant eru...
What happens at the end of the life of massive stars? At one time we thought all these stars followe...
Supernovae are grand and extraordinarily energetic explosions that signify the death of a star. Ther...
Shock-heating of stellar envelopes: A possible common mechanism at the origin of explosions and eru...
How a massive star ends its life depends upon how that life has been lived - the rotation, mass and ...
Explosive astrophysical phenomena have historically played a significant role in understanding the u...
SIGLECopy held by FIZ Karlsruhe; available from UB/TIB Hannover / FIZ - Fachinformationszzentrum Kar...
The impact of rapid rotation of the supernova progenitor star (white dwarf) on its explosion (type I...
Open AccessGamma ray bursts which are first detected in energetic gamma rays and which then glow in ...
SIGLEAvailable from: http://www.mpa-garching.mpg.de / FIZ - Fachinformationszzentrum Karlsruhe / TIB...
Binary star systems known as cataclysmic variables can exhibit violent explosions called novae. Obse...
SIGLEAvailable from: http://www.mpa-garching.mpg.de / FIZ - Fachinformationszzentrum Karlsruhe / TIB...
Durant les dix dernières années, les développements du logiciel d'évolution stellaire de Genève ont ...
SIGLEAvailable from: http://www.mpa-garching.mpg.de / FIZ - Fachinformationszzentrum Karlsruhe / TIB...
In order to deal with dynamical phenomena of stars, gasdynamical equations and, especially, the shoc...
We perform radiation hydrodynamic simulations to study how very massive stars recover from giant eru...