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pro vyhledávání: '"Quentin Pognan"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society
A binary neutron star merger produces a rapidly evolving transient known as a kilonova (KN), which peaks a few days after merger. Modelling of KNe has often been approached assuming local thermodynamic equilibrium (LTE) conditions in the ejecta. We p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::44dbfae6ce798053743c2f6c2cbc65f4
http://arxiv.org/abs/2202.09245
http://arxiv.org/abs/2202.09245
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 492:4058-4079
Accretion onto black holes at rates above the Eddington limit has long been discussed in the context of supermassive black hole (SMBH) formation and evolution, providing a possible explanation for the presence of massive quasars at high redshifts (z$
We use magnetograms of 8 solar analogues of ages 30~Myr to 3.6~Gyr obtained from Zeeman Doppler Imaging (ZDI) and taken from the literature, together with two solar magnetograms, to drive magnetohydrodynamical (MHD) wind simulations and construct an
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a28f99e54671ff05c517401ee45589c3
Publikováno v:
Monthly Notices of the Royal Astronomical Society
The radioactively powered transient following a binary neutron star (BNS) merger, known as a kilonova (KN), is expected to enter the steady-state nebular phase a few days after merger. Steady-state holds until thermal reprocessing time-scales become
Publikováno v:
Astrophysical Journal; 3/20/2018, Vol. 856 Issue 1, p1-1, 1p