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| Indexado |
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| DOI | 10.1051/0004-6361/201322339 | ||||
| Año | 2014 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Results. From the morphology of the inner lobes we conclude that the lobes are not interacting with one another, but are well separated, even at low radio frequencies. We explain the location of the nucleus as the result of the proper motion of the galaxy through the cluster. The required proper motion is of the same order of magnitude as the radial velocity offset of Cygnus A with the sub-cluster it belongs to. The proper motion of the galaxy through the cluster likely also explains the non-colinearity of the jet and counterjet.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | STEENBRUGGE-VAN DEN BERGHE, KATRIEN CHRISTINE | Mujer |
Universidad Católica del Norte - Chile
UNIV OXFORD - Reino Unido University of Oxford - Reino Unido |
| 2 | Blundell, K. M. | Mujer |
UNIV OXFORD - Reino Unido
University of Oxford - Reino Unido |
| 3 | Pyrzas, Stylianos | Hombre |
Universidad Católica del Norte - Chile
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| Fuente |
|---|
| Comisión Nacional de Investigación Científica y Tecnológica |
| ESO |
| Comisión Nacional de Investigación CientÃfica y Tecnológica |
| European School of Oncology |
| ALMA-CONICYT |
| Agradecimiento |
|---|
| K.C.S. and S.P. gratefully acknowledge support from ALMA-CONICYT grant 31110019, and thank ESO for its flexibility (ESO project money could be used till CONICYT transferred the grant several months after the project started). |
| K.C.S. and S.P. gratefully acknowledge support from ALMA-CONICYT grant 31110019, and thank ESO for its flexibility (ESO project money could be used till CONICYT transferred the grant several months after the project started). |