Add to ORKGWe review the effects of winds from massive O and B stars on the surrounding medium over the various stages of stellar evolution. Furthermore we discuss some of the implications for SNe and GRB evolution within this wind-blown medium
Of the cosmological gamma-ray bursts, GRB 011121 has the lowest redshift, z = 0.36. More importantly...
We review the current basic picture of the evolution of massive stars and how their evolution and st...
Massive stars play an important role in both cluster and galactic evolution and the rate at which th...
Most stars will experience episodes of substantial mass loss at some point in their lives. For very ...
The finding of a Type Ic supernova connected with GRB 030329 showed a massive star origin for this b...
Massive stars and supernovae (SNe) have a huge impact on their environment. Despite their importance...
Stars of initial masses between 0.8-8 M☉ will become "asymptotic giant branch" (AGB) stars during th...
A very small fraction of (runaway) massive stars have masses exceeding 60−70M$_⊙$ and are predicted ...
We have investigated the dynamical interaction of low- and-intermediate mass stars (from 1 to 5 Msun...
Stars in the 9-40 solar mass range play a prominent role in the hydrodynamical and chemical evolutio...
Long gamma-ray bursts are highly energetic events that are thought to occur when certain massive sta...
Pulsations driven by partial ionization of hydrogen in the envelope are often considered important f...
We suggest that the mass lost during the evolution of very massive stars may be dominated by optical...
Of the cosmological gamma-ray bursts, GRB 011121 has the lowest redshift, z = 0.36. More importantly...
We study the effect of wind anisotropies on the stellar evolution leading to collapsars. Rotating mo...
Of the cosmological gamma-ray bursts, GRB 011121 has the lowest redshift, z = 0.36. More importantly...
We review the current basic picture of the evolution of massive stars and how their evolution and st...
Massive stars play an important role in both cluster and galactic evolution and the rate at which th...
Most stars will experience episodes of substantial mass loss at some point in their lives. For very ...
The finding of a Type Ic supernova connected with GRB 030329 showed a massive star origin for this b...
Massive stars and supernovae (SNe) have a huge impact on their environment. Despite their importance...
Stars of initial masses between 0.8-8 M☉ will become "asymptotic giant branch" (AGB) stars during th...
A very small fraction of (runaway) massive stars have masses exceeding 60−70M$_⊙$ and are predicted ...
We have investigated the dynamical interaction of low- and-intermediate mass stars (from 1 to 5 Msun...
Stars in the 9-40 solar mass range play a prominent role in the hydrodynamical and chemical evolutio...
Long gamma-ray bursts are highly energetic events that are thought to occur when certain massive sta...
Pulsations driven by partial ionization of hydrogen in the envelope are often considered important f...
We suggest that the mass lost during the evolution of very massive stars may be dominated by optical...
Of the cosmological gamma-ray bursts, GRB 011121 has the lowest redshift, z = 0.36. More importantly...
We study the effect of wind anisotropies on the stellar evolution leading to collapsars. Rotating mo...
Of the cosmological gamma-ray bursts, GRB 011121 has the lowest redshift, z = 0.36. More importantly...
We review the current basic picture of the evolution of massive stars and how their evolution and st...
Massive stars play an important role in both cluster and galactic evolution and the rate at which th...