Zobrazeno 1 - 7
of 7
pro vyhledávání: '"L. A. C. van Son"'
Publikováno v:
The Astrophysical Journal, Vol 966, Iss 1, p 9 (2024)
Chemically homogeneous evolution (CHE) is a promising channel for forming massive binary black holes. The enigmatic, massive Wolf–Rayet binary HD 5980 A&B has been proposed to have formed through this channel. We investigate this claim by comparing
Externí odkaz:
https://doaj.org/article/b0562a6c085e44ef8f3c8c0cafbe7f21
Publikováno v:
The Astrophysical Journal, Vol 948, Iss 2, p 105 (2023)
New observational facilities are probing astrophysical transients such as stellar explosions and gravitational-wave sources at ever-increasing redshifts, while also revealing new features in source property distributions. To interpret these observati
Externí odkaz:
https://doaj.org/article/4e683ac1c88842e98babf378b64c274f
Autor:
L. A. C. van Son, S. E. de Mink, M. Renzo, S. Justham, E. Zapartas, K. Breivik, T. Callister, W. M. Farr, C. Conroy
Publikováno v:
The Astrophysical Journal. 940:184
Gravitational-wave (GW) detections are starting to reveal features in the mass distribution of double compact objects. The lower end of the black hole (BH) mass distribution is especially interesting as few formation channels contribute here and beca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::27e07c793af2067a7727145d70b26fb6
https://doi.org/10.3847/1538-4357/ac9b0a
https://doi.org/10.3847/1538-4357/ac9b0a
Autor:
L. A. C. van Son, S. E. de Mink, T. Callister, S. Justham, M. Renzo, T. Wagg, F. S. Broekgaarden, F. Kummer, R. Pakmor, I. Mandel
Publikováno v:
Astrophysical Journal, 931:17. IOP Publishing Ltd.
Gravitational wave detectors are starting to reveal the redshift evolution of the binary black hole (BBH) merger rate, $R_{\mathrm{BBH}}(z)$. We make predictions for $R_{\mathrm{BBH}}(z)$ as a function of black hole mass for systems originating from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e0859fdd70f44c95ab832f116f8d96d1
http://arxiv.org/abs/2110.01634
http://arxiv.org/abs/2110.01634
Autor:
L. A. C. van Son, K. Chatziioannou, Mathieu Renzo, B. McKernan, Thomas Callister, K. E. S. Ford, Matteo Cantiello, G. Ashton, Chiara M. F. Mingarelli
Understanding common envelope (CE) evolution is an outstanding problem in binary evolution. Although the CE phase is not driven by gravitational-wave (GW) emission, the in-spiraling binary emits GWs that passively trace the CE dynamics. Detecting thi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4b67bf2d56a49abe08a1a6f96ee238f0
https://resolver.caltech.edu/CaltechAUTHORS:20211004-232814510
https://resolver.caltech.edu/CaltechAUTHORS:20211004-232814510
Future searches for gravitational waves from space will be sensitive to double compact objects (DCOs) in our Milky Way. We present new simulations of the populations of double black holes (BHBHs), black hole neutron stars (BHNSs) and double neutron s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::449065be6eb18531e0f23c3c21c48691
Autor:
Robert Farmer, Floor S. Broekgaarden, Stephen Justham, Mathieu Renzo, E. Laplace, D. D. Hendriks, L. A. C. van Son, J. Moran-Fraile, S. E. de Mink
Publikováno v:
Astrophysical Journal, 897(1):100. IOP Publishing Ltd.
The theory for single stellar evolution predicts a gap in the mass distribution of black holes (BHs) between approximately 45-130M$_{\odot}$, the so-called "pair-instability mass gap". We examine whether BHs can pollute the gap after accreting from a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f01ec90b51d6e33b513fd92735bb449a
https://hdl.handle.net/11245.1/cd084181-f20a-446a-8774-9905b1522b2f
https://hdl.handle.net/11245.1/cd084181-f20a-446a-8774-9905b1522b2f