Gamma-ray bursts and black holes. Interpretation of the observational data
| dc.creator | Kuznetsov, A. V. | |
| dc.date | 2001-10-25 | |
| dc.date.accessioned | 2026-07-07T02:01:00Z | |
| dc.date.available | 2026-07-07T02:01:00Z | |
| dc.description | The paper relies upon the (Kuznetsov 2000), where the cosmic gamma - ray bursts (GRBs) in clusters are shown to have an apparent shift relative to the position of the source. Hence the main conclusion follows: only cluster of GRBs ensures correct localization of the source whereas determining the direction of arrival of a single GRB practically carries no information about the position of its source. Generation of repeated GRBs in the activity phase of the source, which amounts to 3-4 months and with the period of repetition of activity equal to 4 years are most general properties of clusters. These properties precisely correspond to the characteristics of manifestation of activity of X-ray NOVAE (BHXN), thus pointing that the source of GRB clusters considered is a black hole (BH) in the XN. The direct identification of the GRB source with the BHXN GRO J0422+32 presented here this confirms. The investigated properties of GRB clusters permit a final solution of 2 main problems of astrophysics: search for black holes and origin of cosmic GRBs. | |
| dc.description | 5 pages, 2 figures | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0110556 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0110556 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/3604 | |
| dc.subject | Astrophysics | |
| dc.title | Gamma-ray bursts and black holes. Interpretation of the observational data | |
| dc.type | text |