INVESTIGADORES
HÄGELE Guillermo Federico
congresos y reuniones científicas
Título:
The jet-cloud interaction in 3CR galaxies
Autor/es:
C. FEINSTEIN, F. D. MACCHETTO, M. F. MONTERO AND G. HÄGELE
Lugar:
La Plata, Buenos Aires, Argentina
Reunión:
Congreso; XLVIII Reunión Anual De La Asociación Argentina de Astronomía; 2005
Institución organizadora:
Facultad de Ciencias Astronómicas y Geofísicas de la Universidad Nacional de La Plata
Resumen:
From the HST/WFPC2 3CR Snapshot Survey, data taken with the filters
F555W, F702W and narrow-ramp, a set of galaxies with noticeable extended
structure were selected (e.g. 3C 79, 3C 135, 3C 234, etc). All of these
objects show large regions of [O III] 5007Å emission (narrow ramp
filter) and the broad-band filters data show similar structures
indicating the presence of strong emission in several lines over these
regions. The morphology observed seems to be related (e.g. same position
angle, direct overlapping or similar shape) with the radio-jet. For some
canditates with this properties GMOS/Gemini
spectrosopy was taken. These data (both HST direct imaging and Gemini
spectroscopy) can be tested with diagnostic diagrams and total UV
photons budget to understand the source of energy that is ionizing the
gas. This source of ionization was commonly believed to be the UV
photons emitted by the powerful AGN, but several of these objects shows
clearly that shocks produce by the radio jet are the main cause of the
observed gas line emission.