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pro vyhledávání: '"Jakob Stegmann"'
Autor:
Jakob Stegmann, Alejandro Vigna-Gómez, Antti Rantala, Tom Wagg, Lorenz Zwick, Mathieu Renzo, Lieke A. C. van Son, Selma E. de Mink, Simon D. M. White
Publikováno v:
The Astrophysical Journal Letters, Vol 972, Iss 2, p L19 (2024)
A substantial fraction of stars can be found in wide binaries with projected separations between ∼10 ^2 and 10 ^5 au. In the standard lore of binary physics, these would evolve as effectively single stars that remotely orbit one another on stationa
Externí odkaz:
https://doaj.org/article/ae1d40135b914cfa9f7c5423ad573e29
Most back hole and neutron star progenitors are found in triples or higher multiplicity systems. Here, we present a new triple stellar evolution code, ${\tt TSE}$, which simultaneously takes into account the physics of the stars and their gravitation
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6dc8f029788b60dd22c8ad13abb64aa1
Publikováno v:
Physical Review D
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 produ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4f04666d81d6ac35d02c912e96bb7ae3
Soon after the recent first ever detection of gravitational waves from merging black holes it has been suggested that their origin is primordial. Appealingly, a sufficient number of primordial black holes (PBHs) could also partially or entirely const
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::847af854a5c7fdcab16bedd4948e88a2
http://arxiv.org/abs/1910.04793
http://arxiv.org/abs/1910.04793