The central radio source in the NGC 383 group: jet - IGM interaction ?
| dc.creator | Komossa, Stefanie | |
| dc.creator | Boehringer, Hans | |
| dc.date | 1999-05-05 | |
| dc.date.accessioned | 2026-07-07T02:31:28Z | |
| dc.date.available | 2026-07-07T02:31:28Z | |
| dc.description | The NGC 383 group is a rich group of galaxies that harbours the central radio source 3C 31 = NGC 383. After presenting results from the X-ray analysis of the extended intra-group medium and the central radio galaxy, we discuss the spatial morphology of X-ray emitting gas as compared to the radio plasma and perform a comparison of the pressures of both components. | |
| dc.description | 4 pages incl. 4 figures (needs ringb99.cls). Contribution to the proc. of the Ringberg workshop on `Diffuse Thermal and Relativistic Plasma in Galaxy Clusters' (Ringberg castle, April 19-23, 1999); to appear as MPE Report. Preprint and related papers also available at http://www.xray.mpe.mpg.de/~skomossa/ | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9905034 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9905034 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14164 | |
| dc.subject | Astrophysics | |
| dc.title | The central radio source in the NGC 383 group: jet - IGM interaction ? | |
| dc.type | text |