Results 41 to 50 of about 63,717 (334)
Gravitational Radiation from Intermediate-Mass Black Holes
Recent X-ray observations of galaxies with ROSAT, ASCA, and Chandra have revealed numerous bright off-center point sources which, if isotropic emitters, are likely to be intermediate-mass black holes, with hundreds to thousands of solar masses.
Benacquista M. +14 more
core +3 more sources
Stellar Mass Black Hole Binaries as ULXs
15 pages, 12 ...
Rappaport, S, Podsiadlowski, P, Pfahl, E
openaire +3 more sources
On the Mass Distribution of Stellar-Mass Black Holes
The observational stellar-mass black hole mass distribution exhibits a maximum at about 8 M⊙. It can be explained via the details of the massive star evolution, supernova explosions, or consequent black hole evolution.
Malkov O. Yu.
doaj +1 more source
A Global Inventory of Feedback
Feedback from both supermassive black holes and massive stars plays a fundamental role in the evolution of galaxies and the inter-galactic medium. In this paper, we use available data to estimate the total amount of kinetic energy and momentum created ...
Timothy M. Heckman, Philip N. Best
doaj +1 more source
Stellar-Mass Black Holes and Their Progenitors
Astro 2010 Science White ...
Miller, J. +16 more
openaire +3 more sources
The Mass Distribution of Stellar Black Holes [PDF]
22 pages including figures, submitted to ...
Bailyn, Charles D. +3 more
openaire +2 more sources
Are stellar-mass binary black hole mergers isotropically distributed? [PDF]
ABSTRACT The Advanced LIGO and Advanced Virgo gravitational wave detectors have detected a population of binary black hole mergers in their first two observing runs. For each of these events, we have been able to associate a potential sky location region represented as a probability distribution on the sky.
Richard Stiskalek +2 more
openaire +2 more sources
Consequences of gravitational radiation recoil [PDF]
Coalescing binary black holes experience an impulsive kick due to anisotropic emission of gravitational waves. We discuss the dynamical consequences of the recoil accompanying massive black hole mergers.
Binggeli B. +9 more
core +3 more sources
Electromagnetic Signals Following Stellar-mass Black Hole Mergers
Abstract It is often assumed that gravitational-wave (GW) events resulting from the merger of stellar-mass black holes are unlikely to produce electromagnetic (EM) counterparts. We point out that the progenitor binary has probably shed a mass ≳10 M ⊙ during its prior evolution.
S. E. de Mink, A. King
openaire +5 more sources
Aims. James Webb Space Telescope (JWST) observations have opened a tantalising new window onto possible black holes as early as redshifts of z ∼ 10.4.
Dayal Pratika, Maiolino Roberto
doaj +1 more source

