We review the current basic picture of the evolution of massive stars and how their evolution and structure changes as a function of initial mass. We give an overview of the fate of modern (Pop I) and primordial (Pop III) stars with emphasis on massive and very massive stars. For single stars we show how the type of explosions, the type of remnant and their frequencies changes for different initial metallicities
The aim of this paper is to look at the evolution of massive stars in order to determine whether or ...
How a massive star ends its life depends upon how that life has been lived - the rotation, mass and ...
The evolution of massive stars in the mass range of 8 to 25 M solar mass is reviewed. The effect of ...
We review the main properties of solar metallicity massive stars in the range 11-120 Msun. The influ...
For the first time, the interior and spectroscopic evolution of a massive star is analyzed from the ...
Publisher's version/PDFCore collapse of dense massive star clusters is unavoidable, and this leads t...
How massive stars die - what sort of explosion and remnant each produces - depends chiefly on the ma...
Massive stars are the ultimate source for nearly all the elements necessary for life. The first star...
Context.We study the evolution and fate of solar composition super-massive stars in the mass range 6...
We show that even most massive initial solar composition stars hardly form black holes with mass exc...
Evolution with moderate mass loss has been investigated for hydrogen-burning stars whose mass exceed...
The first generation of stars is thought to have been very massive (150-300 M�) and produces pair c...
Abstract In this chapter, after a brief introduction and overview of stellar evolu-tion, we discuss ...
While the evolution of massive stars in the local Universe is dominated by mass-loss, the evolution ...
8 pages, 4 figuresWorkshop summaryThe post-main sequence evolution of stars of intermediate or large...
The aim of this paper is to look at the evolution of massive stars in order to determine whether or ...
How a massive star ends its life depends upon how that life has been lived - the rotation, mass and ...
The evolution of massive stars in the mass range of 8 to 25 M solar mass is reviewed. The effect of ...
We review the main properties of solar metallicity massive stars in the range 11-120 Msun. The influ...
For the first time, the interior and spectroscopic evolution of a massive star is analyzed from the ...
Publisher's version/PDFCore collapse of dense massive star clusters is unavoidable, and this leads t...
How massive stars die - what sort of explosion and remnant each produces - depends chiefly on the ma...
Massive stars are the ultimate source for nearly all the elements necessary for life. The first star...
Context.We study the evolution and fate of solar composition super-massive stars in the mass range 6...
We show that even most massive initial solar composition stars hardly form black holes with mass exc...
Evolution with moderate mass loss has been investigated for hydrogen-burning stars whose mass exceed...
The first generation of stars is thought to have been very massive (150-300 M�) and produces pair c...
Abstract In this chapter, after a brief introduction and overview of stellar evolu-tion, we discuss ...
While the evolution of massive stars in the local Universe is dominated by mass-loss, the evolution ...
8 pages, 4 figuresWorkshop summaryThe post-main sequence evolution of stars of intermediate or large...
The aim of this paper is to look at the evolution of massive stars in order to determine whether or ...
How a massive star ends its life depends upon how that life has been lived - the rotation, mass and ...
The evolution of massive stars in the mass range of 8 to 25 M solar mass is reviewed. The effect of ...