EVN Observations of GRS1915+105
| dc.creator | Feretti, L. | |
| dc.creator | Giovannini, G. | |
| dc.creator | Tordi, M. | |
| dc.creator | Venturi, T. | |
| dc.creator | Massaglia, S. | |
| dc.creator | Bodo, G. | |
| dc.creator | Trussoni, E. | |
| dc.creator | Gliozzi, M. | |
| dc.creator | Tavani, M. | |
| dc.creator | Conway, J. | |
| dc.creator | Foley, A. | |
| dc.creator | Graham, D. | |
| dc.creator | Kus, A. | |
| dc.creator | Spencer, R. | |
| dc.creator | Trigilio, C. | |
| dc.date | 2000-09-21 | |
| dc.date | 2000-10-11 | |
| dc.date.accessioned | 2026-07-07T01:55:34Z | |
| dc.date.available | 2026-07-07T01:55:34Z | |
| dc.description | We obtained EVN observations of the X-ray transient source GRS1915+105 in its radio-loud state. In 2 images obtained before a major flare, the source is resolved, showing two opposite asymmetric jets. This indicates that steady jets exist also before a major flare, with an estimated velocity of 0.2-0.6c. | |
| dc.description | Proceedings of the 5th EVN Symposium, Eds. J. Conway, A. Polatidis, R. Booth, Onsala Observatory, Sweden (June 2000) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0009348 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0009348 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/1701 | |
| dc.subject | Astrophysics | |
| dc.title | EVN Observations of GRS1915+105 | |
| dc.type | text |