| dc.creator | GUILLERMO TENORIO TAGLE | |
| dc.creator | SERGIY SILICH | |
| dc.date | 2013-04-01 | |
| dc.date.accessioned | 2023-07-25T16:25:13Z | |
| dc.date.available | 2023-07-25T16:25:13Z | |
| dc.identifier | http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/2233 | |
| dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/7807414 | |
| dc.description | 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. | |
| dc.format | application/pdf | |
| dc.language | eng | |
| dc.publisher | The Astrophysical Journal | |
| dc.relation | citation: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 | |
| dc.rights | info:eu-repo/semantics/openAccess | |
| dc.rights | http://creativecommons.org/licenses/by-nc-nd/4.0 | |
| dc.subject | info:eu-repo/classification/Inspec/Accretion, accretion disks | |
| dc.subject | info:eu-repo/classification/Inspec/Galaxies: active | |
| dc.subject | info:eu-repo/classification/Inspec/Galaxies: star clusters: general | |
| dc.subject | info:eu-repo/classification/Inspec/Hydrodynamics | |
| dc.subject | info:eu-repo/classification/Inspec/Methods: numerical | |
| dc.subject | info:eu-repo/classification/cti/1 | |
| dc.subject | info:eu-repo/classification/cti/21 | |
| dc.subject | info:eu-repo/classification/cti/21 | |
| dc.title | ON THE FATE OF THE MATTER REINSERTED WITHIN YOUNG NUCLEAR STELLAR CLUSTERS | |
| dc.type | info:eu-repo/semantics/article | |
| dc.type | info:eu-repo/semantics/acceptedVersion | |
| dc.audience | students | |
| dc.audience | researchers | |
| dc.audience | generalPublic | |
