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相关论文: Quasars and Galaxy Formation

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When black hole jets encounter ambient medium, they can compress the gas, trigger star formation, and create stellar clusters containing tens of thousands of stars. Here, we report a remarkable discovery of such a phenomenon that happened…

星系天体物理 · 物理学 2025-09-16 Marko Mićić , Themiya Nanayakkara , Xinyu Dai , Jeremy Bailin , Miljan Kolčić

Supermassive black holes have generally been recognized as the most destructive force in nature. But in recent years, they have undergone a dramatic shift in paradigm. These objects may have been critical to the formation of structure in…

天体物理学 · 物理学 2009-09-29 Fulvio Melia

The emergence of the first black holes during the first billion years of cosmic history marks a key event in cosmology. Their formation is part of the overall process of ending the cosmic dark ages, when the first stars appeared in low-mass…

星系天体物理 · 物理学 2019-07-26 Aaron Smith , Volker Bromm

Quasars are widely believed to be powered by accretion onto supermassive black holes and there is now considerable evidence for a link between mergers, quasars and the formation of spheroids. Cattaneo, Haehnelt & Rees (1999) have…

天体物理学 · 物理学 2015-06-24 Andrea Cattaneo

Using axisymmetric simulations coupling special relativistic MHD, an approximate post-Newtonian gravitational potential and two-moment neutrino transport, we show different paths for the formation of either protomagnetars or stellar mass…

太阳与恒星天体物理 · 物理学 2017-05-09 Martin Obergaulinger , Miguel-Ángel Aloy

Supermassive black holes are now realized to exist in the centers of most galaxies. The recent discoveries of luminous quasars at redshifts higher than 6 require that these black holes were assembled already when the Universe was less than…

天体物理学 · 物理学 2009-11-07 H. -Th. Janka

The most massive black holes, lurking at the centers of large galaxies, must have formed less than a billion years after the big bang, as they are visible today in the form of bright quasars at redshift larger than six. Their early…

天体物理学 · 物理学 2009-11-11 M. C. Richter , G. B. Tupper , R. D. Viollier

If the cosmological dark matter has a component made of small primordial black holes, they may have a significant impact on the physics of the first stars and on the subsequent formation of massive black holes. Primordial black holes would…

天体物理学 · 物理学 2009-10-28 Cosimo Bambi , Douglas Spolyar , Alexander D. Dolgov , Katherine Freese , Marta Volonteri

Massive stars have a profound influence on the Universe, but their formation remains poorly understood. We review the current status of observational and theoretical research in this field, describing the various stages of an evolutionary…

天体物理学 · 物理学 2007-05-23 H. Beuther , E. B. Churchwell , C. F. McKee , J. C. Tan

The consequences of nuclear black holes for the structure and dynamics of stellar spheroids are reviewed. Slow growth of a black hole in a pre-existing core produces a steep power-law density profile similar to the cusps seen in faint…

天体物理学 · 物理学 2007-05-23 David Merritt

Primordial black holes (PBHs) may be part of the dark matter. It is shown here that PBHs form more easily during cosmic phase transitions. For approximately scale-invariant primordial curvature fluctuations the PBH mass function may…

宇宙学与河外天体物理 · 物理学 2024-06-18 Karsten Jedamzik

Supermassive black hole accretion and star formation appear intimately connected. I review the observational and theoretical evidence for this statement. I then discuss how focussed studies of two systems, our Galactic Center and the…

天体物理学 · 物理学 2007-05-23 Jonathan C. Tan

The first massive astrophysical black holes likely formed at high redshifts (z>10) at the centers of low mass (~10^6 Msun) dark matter concentrations. These black holes grow by mergers and gas accretion, evolve into the population of bright…

天体物理学 · 物理学 2016-01-27 Zoltan Haiman , Eliot Quataert

The discovery of high redshift quasars represents a challenge to the origin of supermassive black holes. Here, two evolutionary scenarios are considered. The first one concerns massive black holes in the local universe, which in a large…

星系天体物理 · 物理学 2020-01-24 José Antonio de Freitas Pacheco

Young, massive star clusters are the most notable and significant end products of violent star-forming episodes triggered by galaxy collisions, mergers, and close encounters. Their contribution to the total luminosity induced by such…

天体物理学 · 物理学 2009-11-10 Richard de Grijs

We describe the model of protogalaxy formation around the cluster of primordial black holes with a minimum extension of standard cosmological model. Namely, it is supposed, that a mass fraction of the universe ~10^-3 is composed of the…

天体物理学 · 物理学 2007-05-23 Vyacheslav Dokuchaev , Yury Eroshenko , Sergei Rubin

Based on numerical simulations of gas-rich galaxy mergers, we discuss a model in which quasar activity is tied to the self-regulated growth of supermassive black holes in galaxies. Nuclear inflow of gas attending a galaxy collision triggers…

The hypothesis of existence of primordial black holes with large masses (\geq 10^6 M\odot), formed at the earliest stages of the Universe evolution, is considered in the paper. The possibility does not contradict some theories, see e.g.…

宇宙学与河外天体物理 · 物理学 2013-09-17 V. K. Dubrovich , S. I. Glazyrin

Supermassive black holes are found at the centre of massive galaxies. During the growth of these black holes they light up to become visible as active galactic nuclei (AGN) and release extraordinary amounts of energy across the…

星系天体物理 · 物理学 2017-04-26 C. M. Harrison

High redshift quasars mark the locations where massive galaxies are rapidly being assembled and forming stars. There is growing evidence that quasar environments are metal-rich out to redshifts of at least five. The gas-phase metallicities…

天体物理学 · 物理学 2007-05-23 F. Hamann , M. Dietrich , B. Sabra , C. Warner