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pro vyhledávání: '"Mike Y. M. Lau"'
Publikováno v:
The Astrophysical Journal Letters, Vol 966, Iss 1, p L7 (2024)
Accreting main-sequence stars expand significantly when the mass accretion timescale is much shorter than their thermal timescales. This occurs during mass transfer from an evolved giant star onto a main-sequence companion in a binary system and is a
Externí odkaz:
https://doaj.org/article/d57ad713863b4b6aa23a89518c0204df
Autor:
Alejandro Vigna-Gómez, Ilya Mandel, Coenraad J. Neijssel, Mike Y. M. Lau, Alberto Sesana, S. P. Stevenson
Publikováno v:
Lau, M Y M, Mandel, I, Vigna-Gomez, A, Neijssel, C J, Stevenson, S & Sesana, A 2020, ' Detecting double neutron stars with LISA ', Monthly Notices of the Royal Astronomical Society, vol. 492, no. 3, pp. 3061-3072 . https://doi.org/10.1093/mnras/staa002
We estimate the properties of the double neutron star (DNS) population that will be observable by the planned space-based interferometer LISA. By following the gravitational radiation driven evolution of DNSs generated from rapid population synthesis
Autor:
Mike Y M Lau, Ryosuke Hirai, Miguel González-Bolívar, Daniel J Price, Orsola De Marco, Ilya Mandel
We perform 3D hydrodynamical simulations of a common-envelope event involving a 12 solar mass red supergiant donor. Massive stars are expected to be qualitatively different from low-mass stars as their envelopes have significant support from radiatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a633a622327a70f59b40242ee512d4f4