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http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/2233| 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 | |
| Aparece en las colecciones: | Artículos de Astrofísica |
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| 15. On the Fate of the Matter Reinserted within Young Nuclear Stellar Clusters.pdf | 4.68 MB | Adobe PDF | Visualizar/Abrir |