Gravitational Waves Generated by Globular Cluster Systems Collapse
| dc.creator | Capuzzo-Dolcetta, R. | |
| dc.creator | Miocchi, P. | |
| dc.date | 1997-11-06 | |
| dc.date.accessioned | 2026-07-07T02:24:56Z | |
| dc.date.available | 2026-07-07T02:24:56Z | |
| dc.description | According to the hypothesis that AGNs are massive black holes and the mass which feeds them is made of stars belonging to globular clusters frictionally decayed and tidally destroyed by the field of the central object, it is possible to give an estimate of the number and spectral characteristics of detectable gravitational wave impulses generated by the falling of such stars into the black hole. We find that the orbitating gravitational antenna LISA, should detect from 10 to 100 impulses per year. | |
| dc.description | 2 Latex pages + 1 eps figure, epsf.sty and crckapb.sty included; to be published in the Proceedings of the IAU 23rd General Assembly, Symp. 184 "The Central Regions of the Galaxy and Galaxies", Aug 1997, Kyoto, Japan | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9711049 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9711049 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11751 | |
| dc.subject | Astrophysics | |
| dc.title | Gravitational Waves Generated by Globular Cluster Systems Collapse | |
| dc.type | text |