Results 61 to 70 of about 264,425 (308)
Astronomische Nachrichten, Volume 344, Issue 4, May 2023., 2023 Abstract Radiation‐magnetohydrodynamic simulation of the active galactic nuclei predicts the presence of the strong accretion disk wind, which gets unstable far from the central region and turns into gas clumps. These inner wind and outer clumps may be actually observed as the ultrafast outflows (UFOs) and the clumpy absorbers, respectively.
Takuya Midooka +2 more
wiley +1 more source
Universe, 2019 We propose the simple new method for extracting the value of the black hole spin from the direct high-resolution image of black hole by using a thin accretion disk model.
Vyacheslav I. Dokuchaev +1 more
doaj +1 more source
Structure and stability of differentially rotating compact stellar objects
Astronomische Nachrichten, Volume 344, Issue 1-2, January-February 2023., 2023 Abstract Depending on the dynamics of a binary neutron star merger, the collision may result in a differentially rotating compact object. Differentially rotating stars can sustain a total mass considerably higher than that of a uniformly rotating star, giving rise to “hypermassive” objects like hypermassive neutron stars.
Delaney Farrell +2 more
wiley +1 more source
Impact of supermassive black hole growth on star formation [PDF]
Nature Astronomy, 2017 Supermassive black holes are found at the centres of massive galaxies. During the growth of these black holes they light up to become visible as active galactic nuclei (AGNs) and release extraordinary amounts of energy across the electromagnetic spectrum.
C. Harrison, C. Harrison
semanticscholar +1 more source
Key Science Goals for the Next-Generation Event Horizon Telescope
Galaxies, 2023 The Event Horizon Telescope (EHT) has led to the first images of a supermassive black hole, revealing the central compact objects in the elliptical galaxy M87 and the Milky Way.
Michael D. Johnson +44 more
doaj +1 more source
The first supermassive black holes [PDF]
Astronomy & Geophysics, 2017 We briefly review the historical development of the ideas regarding the first supermassive black hole seeds, the physics of their formation and radiative feedback, recent theoretical and observational progress, and our outlook for the future.
Abraham Loeb, Volker Bromm, Aaron Smith
openaire +4 more sources
The distribution of supermassive black holes in the nuclei of nearby galaxies [PDF]
, 1998 The growth of supermassive black holes by merging and accretion in hierarchical models of galaxy formation is studied by means of Monte Carlo simulations.
Cattaneo, A. +4 more
core +4 more sources
Growth of Supermassive Black Holes, Galaxy Mergers and Supermassive Binary Black Holes [PDF]
Proceedings of the International Astronomical Union, 2015 AbstractThe study of galaxy mergers and supermassive binary black holes (SMBBHs) is central to our understanding of the galaxy and black hole assembly and (co-)evolution at the epoch of structure formation and throughout cosmic history. Galaxy mergers are the sites of major accretion episodes, they power quasars, grow supermassive black holes (SMBHs ...
J. G. Baker, F. K. Liu, S. Komossa
openaire +3 more sources
Testing General Relativity with Stellar Orbits around the Supermassive Black Hole in Our Galactic Center. [PDF]
Physical Review Letters, 2017 We demonstrate that short-period stars orbiting around the supermassive black hole in our Galactic center can successfully be used to probe the gravitational theory in a strong regime. We use 19 years of observations of the two best measured short-period
A. Hees +16 more
semanticscholar +1 more source
The spin of supermassive black holes [PDF]
Classical and Quantum Gravity, 2013 Invited article accepted for publication in the focus issue on astrophysical black holes in Classical and Quantum Gravity, guest editors: D. Merritt and L. Rezzolla.
openaire +3 more sources