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A Torus-Dynamo for Magnetic Fields in Galaxies and Accretion Disks

1990
Accretion disks around compact objects as well as the gaseous components in galaxies often have the form of a torus. To study the structure and behaviour of magnetic fields generated in such rings, a kinematic αω-dynamo is investigated which is working inside a torus embedded into vacuum. Modes symmetric and antisymmetric with respect to the equatorial
openaire   +1 more source

Spiral Disk Asymmetries and Other Evidence of Accretion in Nearby Galaxies

1996
Correlations between the stellar disk asymmetries measured in the K-band magnitude, B - V color, residuals from the B-band Tully-Fisher relationship, chemical abundance gradients of nearby spiral galaxies are discussed within the context of a model in which small satellites or H I clouds are accreted onto the outer disks of spiral galaxies.
openaire   +1 more source

The growth of supermassive black holes fed by accretion disks

Astronomy and Astrophysics, 2011
J A De Freitas Pacheco
exaly  

Foundations of Black Hole Accretion Disk Theory

Living Reviews in Relativity, 2013
Marek A Abramowicz   +2 more
exaly  

Accretion disks in luminous young stellar objects

Astronomy and Astrophysics Review, 2016
M T Beltran, W J De Wit
exaly  

Radiation from magnetized accretion disks in AGN

AIP Conference Proceedings, 1992
Robin D Rogers
exaly  

Hydrodynamical activity in thin accretion disks

New Astronomy Reviews, 2008
Oded Regev
exaly  

Do accretion disks exist? IR through radio observations

AIP Conference Proceedings, 1992
Richard Barvainis, Barvainis Richard
exaly  

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