Formation of the first three gravitational-wave observations through isolated binary evolution

Advanced LIGO has detected gravitational waves from two binary black hole mergers, plus a merger candidate. Here the authors use the COMPAS code to show that all three events can be explained by a single evolutionary channel via a common envelope phase, and characterize the progenitor metallicity an...

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Autores principales:	Simon Stevenson, Alejandro Vigna-Gómez, Ilya Mandel, Jim W. Barrett, Coenraad J. Neijssel, David Perkins, Selma E. de Mink
Formato:	article
Lenguaje:	EN
Publicado:	Nature Portfolio 2017
Materias:	Science Q
Acceso en línea:	https://doaj.org/article/fae9ccafe9c64caf841380723559213f
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spelling	oai:doaj.org-article:fae9ccafe9c64caf841380723559213f2021-12-02T15:39:03ZFormation of the first three gravitational-wave observations through isolated binary evolution10.1038/ncomms149062041-1723https://doaj.org/article/fae9ccafe9c64caf841380723559213f2017-04-01T00:00:00Zhttps://doi.org/10.1038/ncomms14906https://doaj.org/toc/2041-1723Advanced LIGO has detected gravitational waves from two binary black hole mergers, plus a merger candidate. Here the authors use the COMPAS code to show that all three events can be explained by a single evolutionary channel via a common envelope phase, and characterize the progenitor metallicity and masses.Simon StevensonAlejandro Vigna-GómezIlya MandelJim W. BarrettCoenraad J. NeijsselDavid PerkinsSelma E. de MinkNature PortfolioarticleScienceQENNature Communications, Vol 8, Iss 1, Pp 1-7 (2017)
institution	DOAJ
collection	DOAJ
language	EN
topic	Science Q
spellingShingle	Science Q Simon Stevenson Alejandro Vigna-Gómez Ilya Mandel Jim W. Barrett Coenraad J. Neijssel David Perkins Selma E. de Mink Formation of the first three gravitational-wave observations through isolated binary evolution
description	Advanced LIGO has detected gravitational waves from two binary black hole mergers, plus a merger candidate. Here the authors use the COMPAS code to show that all three events can be explained by a single evolutionary channel via a common envelope phase, and characterize the progenitor metallicity and masses.
format	article
author	Simon Stevenson Alejandro Vigna-Gómez Ilya Mandel Jim W. Barrett Coenraad J. Neijssel David Perkins Selma E. de Mink
author_facet	Simon Stevenson Alejandro Vigna-Gómez Ilya Mandel Jim W. Barrett Coenraad J. Neijssel David Perkins Selma E. de Mink
author_sort	Simon Stevenson
title	Formation of the first three gravitational-wave observations through isolated binary evolution
title_short	Formation of the first three gravitational-wave observations through isolated binary evolution
title_full	Formation of the first three gravitational-wave observations through isolated binary evolution
title_fullStr	Formation of the first three gravitational-wave observations through isolated binary evolution
title_full_unstemmed	Formation of the first three gravitational-wave observations through isolated binary evolution
title_sort	formation of the first three gravitational-wave observations through isolated binary evolution
publisher	Nature Portfolio
publishDate	2017
url	https://doaj.org/article/fae9ccafe9c64caf841380723559213f
work_keys_str_mv	AT simonstevenson formationofthefirstthreegravitationalwaveobservationsthroughisolatedbinaryevolution AT alejandrovignagomez formationofthefirstthreegravitationalwaveobservationsthroughisolatedbinaryevolution AT ilyamandel formationofthefirstthreegravitationalwaveobservationsthroughisolatedbinaryevolution AT jimwbarrett formationofthefirstthreegravitationalwaveobservationsthroughisolatedbinaryevolution AT coenraadjneijssel formationofthefirstthreegravitationalwaveobservationsthroughisolatedbinaryevolution AT davidperkins formationofthefirstthreegravitationalwaveobservationsthroughisolatedbinaryevolution AT selmaedemink formationofthefirstthreegravitationalwaveobservationsthroughisolatedbinaryevolution
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Formation of the first three gravitational-wave observations through isolated binary evolution

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