Magnetic fields and strong density waves in the interacting galaxy NGC 3627
| dc.creator | Soida, M. | |
| dc.creator | Urbanik, M. | |
| dc.creator | Beck, R. | |
| dc.creator | Wielebinski, R. | |
| dc.date | 1999-04-23 | |
| dc.date.accessioned | 2026-07-07T02:31:21Z | |
| dc.date.available | 2026-07-07T02:31:21Z | |
| dc.description | We present 10.55 GHz observations of strong density-wave spiral NGC 3627. Total power and polarization maps with a resolution of 1.13', sensitive to a weak extended emmision were obtained. In the analysiz we used also available data in the CO ans H_alpha lines. We present simple modelling results showing the imprtance of large-scale dynamo-type magnetic field present despite the strong density-wave action in this galaxy. | |
| dc.description | 10 pages (including 10 figures); A&A accepted (1999) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9904323 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9904323 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14125 | |
| dc.subject | Astrophysics | |
| dc.title | Magnetic fields and strong density waves in the interacting galaxy NGC 3627 | |
| dc.type | text |