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quasars: supermassive black holes

A Unified, Merger‐driven Model of the Origin of Starbursts, Quasars, the Cosmic X‐Ray Background, Supermassive Black Holes, and Galaxy Spheroids

A Unified, Merger‐driven Model of the Origin of Starbursts, Quasars, the Cosmic X‐Ray Background, Supermassive Black Holes, and Galaxy Spheroids

... permassive black holes represent connected phases in the lives of ...of supermassive black ...a black hole dominates the energetics of the central region, feedback expels gas and dust, ...

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A Cosmological Framework for the Co‐evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies. I. Galaxy Mergers and Quasar Activity

A Cosmological Framework for the Co‐evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies. I. Galaxy Mergers and Quasar Activity

... efficient. We contrast this with a secular model in which quasar activity is driven by bars or other disk insta- bilities, and show that while these modes of fueling probably dominate the high-Eddington ratio population ...

35

A Cosmological Framework for the Co‐evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies. II. Formation of Red Ellipticals

A Cosmological Framework for the Co‐evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies. II. Formation of Red Ellipticals

... bursts, quasars, and red galaxies as different phases of the same events, we can graft these simulations onto our theoreti- cal, cosmological calculation and determine the cosmological birthrate of these various ...

31

Bonoli, Silvia
  

(2010):


	The Role of Galaxy Mergers in the Evolution of Supermassive Black Holes.


Dissertation, LMU München: Fakultät für Physik

Bonoli, Silvia (2010): The Role of Galaxy Mergers in the Evolution of Supermassive Black Holes. Dissertation, LMU München: Fakultät für Physik

... massive black holes, from the time when the first stars were formed to the Universe we see ...with black hole growth and its interaction with the host galaxy are still ...of black hole ...

147

An Upper Limit to the Degree of Evolution between Supermassive Black Holes and Their Host Galaxies

An Upper Limit to the Degree of Evolution between Supermassive Black Holes and Their Host Galaxies

... All of these predictions appear to be opposite the ob- servations, with quasar spectra dominated by post-starburst activity (Vanden Berk et al. 2006), typically early-type, bulge-dominated hosts (especially in the ...

7

Tidal disruption of stars by supermassive black holes: The X-ray view

Tidal disruption of stars by supermassive black holes: The X-ray view

... – TDEs are markers of recoiling SMBHs. Tidal disruptions of stars in the star cluster bound to an ejected SMBH after GW recoil will produce off-center (or even intergalactic) flares of quasar-like luminosity, and in that ...

7

Monsters on the Move: Gravitational Recoil of Supermassive Black Holes in Nearby Elliptical Galaxies

Monsters on the Move: Gravitational Recoil of Supermassive Black Holes in Nearby Elliptical Galaxies

... radio-loud quasars (RLQs), for example, Hutchings and Neff (1991) have found that the host galaxy is red, featureless and very large, with an es- timated diameter of 75 kpc (∼ 24”), which suggests an elliptical ...

148

Supermassive Black Holes, Large Scale Structure and Holography

Supermassive Black Holes, Large Scale Structure and Holography

... In the earliest phase of development of large scale structure, at z  6 , there was only one Jeans’ mass struc- ture level in the holographic model for large scale struc- ture [2]. These earliest large scale structures, ...

5

Eisenreich, Maximilian
  

(2018):


	Supermassive black holes and multiphase gas in early-type galaxies.


Dissertation, LMU München: Fakultät für Physik

Eisenreich, Maximilian (2018): Supermassive black holes and multiphase gas in early-type galaxies. Dissertation, LMU München: Fakultät für Physik

... a black hole works in detail is still a topic of ongoing research, complicated by the small scales and extreme conditions under which it takes ...the black hole (Shakura & Sunyaev, ...(e.g. ...

195

Formation of Galaxies in the Context of Gravitational Waves and Primordial Black Holes

Formation of Galaxies in the Context of Gravitational Waves and Primordial Black Holes

... of black holes at the center of galaxies is a promising chan- nel for a better understanding of galaxy formation ...detected supermassive black holes with masses in excess of one ...

11

The growth of typical star-forming galaxies and their supermassive black holes across cosmic time since z ~ 2

The growth of typical star-forming galaxies and their supermassive black holes across cosmic time since z ~ 2

... Current studies cannot establish whether or not radiatively driven winds have a significant effect on a galactic scale. Integral field unit observations provide evidence for outflowing gas in local Seyferts (e.g. Davies ...

9

Dark Matter Halo Mergers and Quasars

Dark Matter Halo Mergers and Quasars

... the supermassive black holes they harbor at their nuclei depends strongly on the merger history of their surrounding dark matter ...individual quasars. In this model, the mass of the seed ...

373

Black hole physics destruction phase of universe  (1) big bang only do discuss expansion phase, destruction phase not yet investigated

Black hole physics destruction phase of universe (1) big bang only do discuss expansion phase, destruction phase not yet investigated

... massive black holes, which would explain why they are the brightest objects in the ...distant quasars, found at high redshifts of ...that quasars are embedded in massive host ...two ...

20

Supermassive Black Holes

Supermassive Black Holes

... following black hole model, electrons and positrons form a neutral gas which is confined by ...of black holes, for the range 1000 to 100 billion solar ...

5

Rebusco, Paola
  

(2007):


	Impact of supermassive black holes on galaxy clusters.


Dissertation, LMU München: Fakultät für Physik

Rebusco, Paola (2007): Impact of supermassive black holes on galaxy clusters. Dissertation, LMU München: Fakultät für Physik

... time – a factor of 10 to 100 shorter than the Hubble time. Recent X-ray observations (e.g. Peterson et al. 2003, Matsushita et al. 2002, Kaastra et al. 2004) however suggest that the gas does not cool below temperatures ...

143

EHT Constraint on the Ultralight Scalar Hair of the M87 Supermassive Black Hole

EHT Constraint on the Ultralight Scalar Hair of the M87 Supermassive Black Hole

... for supermassive BHs, such as the one recently observed by the Event Horizon Telescope (EHT) collaboration [14–16] at the centre of the supergiant elliptic galaxy M87, henceforth referred to as the M87 ...

13

On the Origin of the Gamma Ray Burst  Redshift Distribution in the Early Universe

On the Origin of the Gamma Ray Burst Redshift Distribution in the Early Universe

... Black holes in the early universe were formed via various channels that depend on the local environment reign- ing in ...a black hole ...a black hole [26] [27]. The final mass of the newly ...

5

How frequent are close supermassive binary black holes in powerful jet sources?

How frequent are close supermassive binary black holes in powerful jet sources?

... Similar to Hydra A, Cen A is also a source with S-symmetric struc- ture (Fig. C1, Morganti et al. 1999b). The inner structure has a size and geometry very similar to Hydra A, suggesting also a precession with period of ...

22

Black Holes—Information Models

Black Holes—Information Models

... the black hole is proportional to its squared ...a black hole contains pairwise interacting particles ...the black hole on its mass can be explained by the fact that each interaction forms 1 bit of ...

13

Preons, Gravity and Black Holes

Preons, Gravity and Black Holes

... of black holes, the role of rotational curvature, or gravitons, at Planck scale is traditionally to give the radius-mass relation of the black hole ...

17

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