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ON THE FATE OF THE MATTER REINSERTED WITHIN YOUNG NUCLEAR STELLAR CLUSTERS | |
GUILLERMO TENORIO TAGLE SERGIY SILICH | |
Acceso Abierto | |
Atribución-NoComercial-SinDerivadas | |
Accretion, accretion disks Galaxies: active Galaxies: star clusters: general Hydrodynamics Methods: numerical | |
This paper presents a hydrodynamical model describing the evolution of the gas reinserted by stars within a rotating young nuclear star cluster (NSC). We explicitly consider the impact of the stellar component on the flow by means of a uniform insertion of mass and energy within the stellar cluster. The model includes the gravity force of the stellar component and a central supermassive black hole (SMBH), and accounts for the heating from the central source of radiation and the radiative cooling of the thermalized gas. By using a set of parameters typical for NSCs and SMBHs in Seyfert galaxies, our simulations show that a filamentary/clumpy structure is formed in the inner part of the cluster. This “torus” is Compton-thick and covers a large fraction of the sky (as seen from the SMBH).In the outer parts of the cluster a powerful wind is produced that inhibits the infall of matter from larger scales andthus the NSC–SMBH interplay occurs in isolation. | |
The Astrophysical Journal | |
01-04-2013 | |
Artículo | |
Inglés | |
Estudiantes Investigadores Público en general | |
Hueyotl-Zahuantitla, Filiberto, et al., (2013). ON THE FATE OF THE MATTER REINSERTED WITHIN YOUNG NUCLEAR STELLAR CLUSTERS, The Astrophysical Journal, Vol. 766(92):1-11 | |
ASTRONOMÍA Y ASTROFÍSICA | |
Versión aceptada | |
acceptedVersion - Versión aceptada | |
Appears in Collections: | Artículos de Astrofísica |
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