Add to ORKGSome 10% of all massive stars are predicted to merge completely with a companion star. Here we review the different types of mergers and how they may produce unusual objects such as the anomalous progenitor of SN 1987A, gamma-ray burst sources and Thorne-Zytkow objects
We study close encounters involving massive main sequence stars and the evolution of the exotic prod...
We present a model for the formation of high-mass close binary systems in the context of forming mas...
The VLT-FLAMES Tarantula Survey is an ESO Large Program from which we have obtained multi-epoch opti...
Some 10% of all massive stars are predicted to merge completely with a companion star. Here we revie...
Since the majority of massive stars are members of binary systems, an understanding of the intricaci...
The presence of a nearby companion alters the evolution of massive stars in binary systems, leading ...
The presence of a nearby companion alters the evolution of massive stars in binary systems, leading ...
The presence of a nearby companion alters the evolution of massive stars in binary systems, leading ...
Because the majority of massive stars are born as members of close binary systems, populations of ma...
The nature of the progenitor has been one of the major mysteries of SN 1987A. It has long been suspe...
This thesis studies the origin of two exotic stellar phenomena from the merger of binary stars: Sup...
We study the complete merger of two massive stars inside a common envelope and the subsequent evolut...
We study the complete merger of two massive stars inside a common envelope and the subsequent evolut...
As many young massive stars are found in close binaries, many core-collapse supernova progenitors ar...
We present the results of a systematic study of how the CNO abundances in the envelopes of massive s...
We study close encounters involving massive main sequence stars and the evolution of the exotic prod...
We present a model for the formation of high-mass close binary systems in the context of forming mas...
The VLT-FLAMES Tarantula Survey is an ESO Large Program from which we have obtained multi-epoch opti...
Some 10% of all massive stars are predicted to merge completely with a companion star. Here we revie...
Since the majority of massive stars are members of binary systems, an understanding of the intricaci...
The presence of a nearby companion alters the evolution of massive stars in binary systems, leading ...
The presence of a nearby companion alters the evolution of massive stars in binary systems, leading ...
The presence of a nearby companion alters the evolution of massive stars in binary systems, leading ...
Because the majority of massive stars are born as members of close binary systems, populations of ma...
The nature of the progenitor has been one of the major mysteries of SN 1987A. It has long been suspe...
This thesis studies the origin of two exotic stellar phenomena from the merger of binary stars: Sup...
We study the complete merger of two massive stars inside a common envelope and the subsequent evolut...
We study the complete merger of two massive stars inside a common envelope and the subsequent evolut...
As many young massive stars are found in close binaries, many core-collapse supernova progenitors ar...
We present the results of a systematic study of how the CNO abundances in the envelopes of massive s...
We study close encounters involving massive main sequence stars and the evolution of the exotic prod...
We present a model for the formation of high-mass close binary systems in the context of forming mas...
The VLT-FLAMES Tarantula Survey is an ESO Large Program from which we have obtained multi-epoch opti...