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Impact of massive binary star and cosmic evolution on gravitational wave observations I

Autor: S. P. Stevenson, Ilya Mandel, Alejandro Vigna-Gómez, Edo Berger, Stephen Justham, Debatri Chattopadhyay, Floor S. Broekgaarden, Martyna Chruslinska, Selma E. de Mink, Coenraad J. Neijssel

Publikováno v: Monthly Notices of the Royal Astronomical Society, 508(4), 5028-5063. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 508, 4, pp. 5028-5063
Broekgaarden, F S, Berger, E, Neijssel, C J, Vigna-Gomez, A, Chattopadhyay, D, Stevenson, S, Chruslinska, M, Justham, S, de Mink, S E & Mandel, I 2021, ' Impact of massive binary star and cosmic evolution on gravitational wave observations I : black hole-neutron star mergers ', Monthly Notices of the Royal Astronomical Society, vol. 508, no. 4, pp. 5028-5063 . https://doi.org/10.1093/mnras/stab2716
Monthly Notices of the Royal Astronomical Society, 508, 5028-5063

Mergers of black hole-neutron star (BHNS) binaries have now been observed by GW detectors with the recent announcement of GW200105 and GW200115. Such observations not only provide confirmation that these systems exist, but will also give unique insig

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cd2cd08e44098dc868e748760b7bcbc3
https://dare.uva.nl/personal/pure/en/publications/impact-of-massive-binary-star-and-cosmic-evolution-on-gravitational-wave-observations-i(3d86099b-024e-46ec-82e0-4d28b204b9b4).html

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Luminous Red Novae: population models and future prospects

Autor: Coenraad J. Neijssel, Simon Stevenson, Ilya Mandel, Stephen Justham, G. Howitt, Tyrone E. Woods, Alejandro Vigna-Gómez, N. Ivanova

Publikováno v: Howitt, G, Stevenson, S, Vigna-Gomez, A, Justham, S, Ivanova, N, Woods, T E, Neijssel, C J & Mandel, I 2020, ' Luminous Red Novae : population models and future prospects ', Monthly Notices of the Royal Astronomical Society, vol. 492, no. 3, pp. 3229-3240 . https://doi.org/10.1093/mnras/stz3542
Monthly Notices of the Royal Astronomical Society, 492(3), 3229-3240. Oxford University Press

A class of optical transients known as Luminous Red Novae (LRNe) have recently been associated with mass ejections from binary stars undergoing common-envelope evolution. We use the population synthesis code COMPAS to explore the impact of a range of

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::602f43884c8ff7c9556ee13786962b9a
https://doi.org/10.1093/mnras/stz3542

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Stellar response after stripping as a model for common-envelope outcomes

Autor: Alejandro Vigna-Gómez, Michelle Wassink, Jakub Klencki, Alina Istrate, Gijs Nelemans, Ilya Mandel

Publikováno v: Monthly Notices of the Royal Astronomical Society, 511, 2, pp. 2326-2338
Vigna-Gomez, A, Wassink, M, Klencki, J, Istrate, A, Nelemans, G & Mandel, I 2022, ' Stellar response after stripping as a model for common-envelope outcomes ', Monthly Notices of the Royal Astronomical Society, vol. 511, no. 2, pp. 2326-2338 . https://doi.org/10.1093/mnras/stac237
Monthly Notices of the Royal Astronomical Society, 511, 2326-2338

Binary neutron stars have been observed as millisecond pulsars, gravitational-wave sources, and as the progenitors of short gamma-ray bursts and kilonovae. Massive stellar binaries that evolve into merging double neutron stars are believed to experie

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e48de4e425ac179a4591cc807f694ca6
http://arxiv.org/abs/2107.14526

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