Binary black hole mergers from merged stars in the Galactic field

The majority of massive stars are found in close binaries which: (i) are prone to merge and (ii) are accompanied by another distant tertiary star (triples). Here, we study the evolution of the stellar post-merger binaries composed of the merger product and the tertiary companion. We find that post-m...

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Main Authors: Stegmann, Jakob (Author) , Antonini, Fabio (Author) , Schneider, Fabian (Author) , Tiwari, Vaibhav (Author) , Chattopadhyay, Debatri (Author)
Format: Article (Journal) Chapter/Article
Language:English
Published: 27 Jun 2022
Edition:Version v2
In: Arxiv
Year: 2022, Pages: 1-13
DOI:10.48550/arXiv.2203.16544
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.48550/arXiv.2203.16544
Verlag, lizenzpflichtig, Volltext: http://arxiv.org/abs/2203.16544
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Author Notes:Jakob Stegmann, Fabio Antonini, Fabian R.N. Schneider, Vaibhav Tiwari, and Debatri Chattopadhyay
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Binary black hole mergers from merged stars in the Galactic field by Stegmann, Jakob (Author) , Antonini, Fabio (Author) , Schneider, Fabian (Author) , Tiwari, Vaibhav (Author) , Chattopadhyay, Debatri (Author) ,


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