The VLBI morphology of M81* at 43 GHz
| dc.creator | Ros, Eduardo | |
| dc.creator | Perez-Torres, Miguel-Angel | |
| dc.date | 2008-11-26 | |
| dc.date.accessioned | 2026-07-07T12:04:48Z | |
| dc.date.available | 2026-07-07T12:04:48Z | |
| dc.description | The radio source M81* at the core of the nearby spiral galaxy M81 is a low-luminosity active galactic nucleus. The close distance of 3.63Mpc allows its morphology to be studied in great detail. Here we present preliminary results from continuum 7 mm VLBI observations of its core, using phase-referencing techniques. These observations set constrains on the size of M81* at this frequency and enable us to test the frequency dependence on its physical properties. | |
| dc.description | Proceedings of Science, Proc. of the 9th European VLBI Network Symposium on the Role of VLBI in the Golden Age for Radio Astronomy and EVN Users Meeting, Bologna, September 2008; 3 pages, 1 figure, needs PoS.cls | |
| dc.identifier | https://arxiv.org/abs/0811.4340 | |
| dc.identifier | http://arxiv.org/abs/0811.4340 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/208210 | |
| dc.subject | Astrophysics | |
| dc.title | The VLBI morphology of M81* at 43 GHz | |
| dc.type | text |