scholarly journals Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger

2014 ◽  
Vol 441 (4) ◽  
pp. 3444-3453 ◽  
Author(s):  
Brian D. Metzger ◽  
Rodrigo Fernández
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Hole Formation ◽  
Black Hole Formation

scholarly journals Systematics of prompt black-hole formation in neutron star mergers

2021 ◽  
Vol 103 (12) ◽  
Author(s):  
Andreas Bauswein ◽  
Sebastian Blacker ◽  
Georgios Lioutas ◽  
Theodoros Soultanis ◽  
Vimal Vijayan ◽  
...  
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Hole Formation ◽  
Black Hole Formation

scholarly journals Inferring prompt black-hole formation in neutron star mergers from gravitational-wave data

2020 ◽  
Vol 101 (4) ◽  
Author(s):  
Michalis Agathos ◽  
Francesco Zappa ◽  
Sebastiano Bernuzzi ◽  
Albino Perego ◽  
Matteo Breschi ◽  
...  
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Gravitational Wave ◽  
Hole Formation ◽  
Black Hole Formation ◽  
Wave Data

scholarly journals GRB 140619B: A SHORT GRB FROM A BINARY NEUTRON STAR MERGER LEADING TO BLACK HOLE FORMATION

2015 ◽  
Vol 808 (2) ◽  
pp. 190 ◽  
Author(s):  
R. Ruffini ◽  
M. Muccino ◽  
M. Kovacevic ◽  
F. G. Oliveira ◽  
J. A. Rueda ◽  
...  
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Hole Formation ◽  
Black Hole Formation ◽  
Binary Neutron Star

scholarly journals GRB 140619B: a short GRB from a neutron star merger leading to the black hole formation

2015 ◽  
Author(s):  
Marco Muccino ◽  
Remo Ruffini ◽  
Milos Kovacevic ◽  
Luca Izzo ◽  
Fernanda G. Oliveira ◽  
...  
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Hole Formation ◽  
Black Hole Formation

scholarly journals GRB 140619B: A short GRB from a binary neutron star merger leading to black hole formation

2017 ◽  
Author(s):  
Marco Muccino ◽  
R. Ruffini ◽  
Milos Kovacevic ◽  
Fernanda G. Oliveira ◽  
Jorge A. Rueda ◽  
...  
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Hole Formation ◽  
Black Hole Formation ◽  
Binary Neutron Star

scholarly journals Feeding and feedback from little monsters: AGN in dwarf galaxies

2020 ◽  
Vol 15 (S359) ◽  
pp. 238-242
Author(s):  
Mar Mezcua
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Early Universe ◽  
Dwarf Galaxies ◽  
Scaling Relations ◽  
Strong Impact ◽  
Hole Formation ◽  
Intermediate Mass ◽  
Black Hole Formation ◽  
Low Mass

AbstractDetecting the seed black holes from which quasars formed is extremely challenging; however, those seeds that did not grow into supermassive should be found as intermediate-mass black holes (IMBHs) of 100 – 105 M⊙ in local dwarf galaxies. The use of deep multiwavelength surveys has revealed that a population of actively accreting IMBHs (low-mass AGN) exists in dwarf galaxies at least out to z ˜3. The black hole occupation fraction of these galaxies suggests that the early Universe seed black holes formed from direct collapse of gas, which is reinforced by the possible flattening of the black hole-galaxy scaling relations at the low-mass end. This scenario is however challenged by the finding that AGN feedback can have a strong impact on dwarf galaxies, which implies that low-mass AGN in dwarf galaxies might not be the untouched relics of the early seed black holes. This has important implications for seed black hole formation models.

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