A detailed study of the nuclear region of Mrk 273
| dc.creator | Bondi, M. | |
| dc.creator | Dallacasa, D. | |
| dc.creator | Torres, M. A. Peerez | |
| dc.creator | Muxlow, T. W. B. | |
| dc.date | 2004-12-29 | |
| dc.date.accessioned | 2026-07-07T02:16:29Z | |
| dc.date.available | 2026-07-07T02:16:29Z | |
| dc.description | We present 5 GHz EVN+MERLIN observations of the nuclear region of the ultra luminous infrared galaxy Mrk 273. These observations confirms the detection, on the mas scale, of two resolved component labelled as N and SE in the literature. We use published VLBA observations at 1.4 GHz, at the same resolution, to derive spectral index information of component N and SE and discuss these findings in relation with different hypothesis (compact starburst or AGN) for the origin of the radio emission. | |
| dc.description | 4 pages. 6 figures. Proceedings of the 7th European VLBI Network Symposium held in Toledo, Spain on October 12-15, 2004. Editors: R. Bachiller, F. Colomer, J.-F. Desmurs, P. de Vicente (Observatorio Astronomico Nacional), p. 121-124. Needs evn2004.cls | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0412659 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0412659 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/8803 | |
| dc.subject | Astrophysics | |
| dc.title | A detailed study of the nuclear region of Mrk 273 | |
| dc.type | text |