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...

Celý popis

Uložené v:

Podrobná bibliografia
Vydané v:	Monthly notices of the Royal Astronomical Society Ročník 403; číslo 4; s. 1801 - 1811
Hlavní autori:	Schartmann, M., Burkert, A., Krause, M., Camenzind, M., Meisenheimer, K., Davies, R. I.
Médium:	Journal Article
Jazyk:	English
Vydavateľské údaje:	Oxford, UK Blackwell Publishing Ltd 21.04.2010 Wiley-Blackwell Oxford University Press
Predmet:	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
On-line prístup:	Získať plný text
Tagy:	Pridať tag Žiadne tagy, Buďte prvý, kto otaguje tento záznam!

Buďte prvý, kto okomentuje tento záznam!