Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Lieke A C van Son"'
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
Autor:
Floor S Broekgaarden, Edo Berger, Simon Stevenson, Stephen Justham, Ilya Mandel, Martyna Chruślińska, Lieke A C van Son, Tom Wagg, Alejandro Vigna-Gómez, Selma E de Mink, Debatri Chattopadhyay, Coenraad J Neijssel
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 516, 4, pp. 5737-5761
Monthly Notices of the Royal Astronomical Society, 516, 5737-5761
Broekgaarden, F S, Berger, E, Stevenson, S, Justham, S, Mandel, I, Chruslinska, M, van Son, L A C, Wagg, T, Vigna-Gomez, A, de Mink, S E, Chattopadhyay, D & Neijssel, C J 2022, ' Impact of massive binary star and cosmic evolution on gravitational wave observations-II. Double compact object rates and properties ', Monthly Notices of the Royal Astronomical Society, vol. 516, no. 4, pp. 5737-5761 . https://doi.org/10.1093/mnras/stac1677
Monthly Notices of the Royal Astronomical Society, 516, 5737-5761
Broekgaarden, F S, Berger, E, Stevenson, S, Justham, S, Mandel, I, Chruslinska, M, van Son, L A C, Wagg, T, Vigna-Gomez, A, de Mink, S E, Chattopadhyay, D & Neijssel, C J 2022, ' Impact of massive binary star and cosmic evolution on gravitational wave observations-II. Double compact object rates and properties ', Monthly Notices of the Royal Astronomical Society, vol. 516, no. 4, pp. 5737-5761 . https://doi.org/10.1093/mnras/stac1677
Making the most of the rapidly increasing population of gravitational-wave detections of black hole (BH) and neutron star (NS) mergers requires comparing observations with population synthesis predictions. In this work we investigate the combined imp
Autor:
Rohan P. Naidu, Alexander P. Ji, Charlie Conroy, Ana Bonaca, Yuan-Sen Ting, Dennis Zaritsky, Lieke A. C. van Son, Floor S. Broekgaarden, Sandro Tacchella, Vedant Chandra, Nelson Caldwell, Phillip Cargile, Joshua S. Speagle
Publikováno v:
The Astrophysical Journal Letters. 926:L36
The astrophysical origins of $r$-process elements remain elusive. Neutron star mergers (NSMs) and special classes of core-collapse supernovae (rCCSNe) are leading candidates. Due to these channels' distinct characteristic timescales (rCCSNe: prompt,