Gas dynamics of the central few parsec region of NGC 1068 fuelled by the evolving nuclear star cluster

Recently, high-resolution observations with the help of the near-infrared adaptive optics integral field spectrograph Spectrograph for INtegral Field Observations in the Near Infrared (SINFONI) at the Very Large Telescope proved the existence of massive and young nuclear star clusters in the centres...

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Bibliographic Details
Published in:	Monthly notices of the Royal Astronomical Society Vol. 403; no. 4; pp. 1801 - 1811
Main Authors:	Schartmann, M., Burkert, A., Krause, M., Camenzind, M., Meisenheimer, K., Davies, R. I.
Format:	Journal Article
Language:	English
Published:	Oxford, UK Blackwell Publishing Ltd 21.04.2010 Wiley-Blackwell Oxford University Press
Subjects:	accretion accretion discs accretion, accretion discs Astronomy Astrophysics Earth, ocean, space Exact sciences and technology galaxies: nuclei galaxies: Seyfert galaxies: structure hydrodynamics ISM: evolution Simulation Spectrum analysis Stars & galaxies galaxies: structure galaxies: Seyfert hydrodynamics galaxies: nuclei ISM: evolution accretion, accretion discs Young cluster Seyfert 2 galaxies Accretion disks Interferometric observation Young stars Seyfert galaxies Momentum transfer Star formation Galaxy nuclei Turbulent viscosity Observables Age Pluto planet Nuclear cluster model Turbulence Radial distribution Gas dynamics Digital simulation Mass loss Star clusters Density distribution Mass transfer Stellar mass Galaxy structure Tori Rotating disk Masers Angular momentum Hydrodynamic model Adaptive optics Interstellar matter
ISSN:	0035-8711, 1365-2966
Online Access:	Get full text
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