Zobrazeno 1 - 10
of 157
pro vyhledávání: '"Bever, J."'
Publikováno v:
In Surface & Coatings Technology 30 October 2024 494 Part 2
Publikováno v:
A&A 636, A99 (2020)
Theoretical population number studies of binaries with at least one black hole (BH) component are obviously depending on whether or not BHs receive a (natal) kick during their formation. Several observational facts seem to indicate that indeed BHs re
Externí odkaz:
http://arxiv.org/abs/1912.01256
We first summarize work that has been done on the effects of binaries on theoretical population synthesis of stars and stellar phenomena. Next, we highlight the influence of stellar dynamics in young clusters by discussing a few candidate UFOs (uncon
Externí odkaz:
http://arxiv.org/abs/0801.2674
Publikováno v:
Astrophys.Space Sci.324:271-276,2009
In the present paper we combine an N-body code that simulates the dynamics of young dense stellar systems with a massive star evolution handler that accounts in a realistic way for the effects of stellar wind mass loss. We discuss two topics: 1. The
Externí odkaz:
http://arxiv.org/abs/0712.3343
The early evolution of dense stellar systems is governed by massive single star and binary evolution. Core collapse of dense massive star clusters can lead to the formation of very massive objects through stellar collisions ($M\geq$ 1000 \msun). Stel
Externí odkaz:
http://arxiv.org/abs/0710.1752
We discuss differences between massive single star and massive close binary population number synthesis predictions of WR stars. We show that the WC/WN number ratio as function of metallicity depends significantly on whether or not binaries are inclu
Externí odkaz:
http://arxiv.org/abs/astro-ph/0703796
Publikováno v:
Astrophys.J.659:1576-1581,2007
Core collapse of dense massive star clusters is unavoidable and this leads to the formation of massive objects, with a mass up to 1000 $\msun$ and even larger. When these objects become stars, stellar wind mass loss determines their evolution and fin
Externí odkaz:
http://arxiv.org/abs/astro-ph/0701334
In the present paper we report on first results of a project in Brussels where we study the effects of stellar dynamics on the evolution of young dense stellar systems using the 3 decades expertise in massive star evolution and our population (number
Externí odkaz:
http://arxiv.org/abs/astro-ph/0410510
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