Predicting gravitational wave signals from BPASS white dwarf binary and black hole binary populations of a Milky Way-like galaxy model for LISA

被引：0
|
作者：
Tang, P. [1 ]
Eldridge, J.J. [1 ]
Meyer, R. [2 ]
Lamberts, A. [3 ,4 ]
Boileau, G. [5 ]
van Zeist, W.G.J. [1 ,6 ,7 ]
机构：
[1] Department of Physics, University of Auckland, Private Bag 92019, Auckland, New Zealand
[2] Department of Statistics, University of Auckland, Private Bag 92019, Auckland, New Zealand
[3] Observatoire de la Côte d’Azur, Université Côte d’Azur, CNRS, Laboratoire Lagrange, Bd de l’Observatoire, Nice,F-06304, France
[4] Observatoire de la Côte d’Azur, Université Côte d’Azur, CNRS, Artemis, Bd de l’Observatoire, Nice,F-06304, France
[5] Department of Physics, University of Antwerpen, Prinsstraat 13, Antwerpen,2000, Belgium
[6] Department of Astrophysics, IMAPP, Radboud University, PO Box 9010, Nijmegen,6500 GL, Netherlands
[7] Leiden Observatory, Leiden University, PO Box 9513, Leiden,2300 RA, Netherlands
来源：
Monthly Notices of the Royal Astronomical Society | 2024年 / 534卷 / 03期
关键词：
(star:) white dwarf - Binaries:general - Black holes - Dwarf binaries - Galaxy:stellar content - Gravitational-waves - Population synthesis - Spectral synthesis - Stars: black holes - Stars: white dwarf;
D O I：
10.1093/mnras/stae2154
中图分类号：
学科分类号：
摘要：
95
引用
收藏
页码：1707 / 1728
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