IAR   05382
INSTITUTO ARGENTINO DE RADIOASTRONOMIA
Unidad Ejecutora - UE
artículos
Título:
Subarcsecond radio continuum mapping in and around the spiral galaxy NGC3351 using MERLIN
Autor/es:
HÄGELE, GUILLERMO F.; ASCASIBAR, YAGO; RICHARDS, ANITA M. S.; CARDACI, MÓNICA V.; VÁSQUEZ, JAVIER; DÍAZ, ÁNGELES I.; ROSA GONZÁLEZ, DANIEL; TERLEVICH, ROBERTO; TERLEVICH, ELENA
Revista:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Editorial:
WILEY-BLACKWELL PUBLISHING, INC
Referencias:
Año: 2010 vol. 406 p. 1675 - 1686
ISSN:
0035-8711
Resumen:
We report subarcsecond-scale radio continuum observations of a field of
35 × 22 arcmin2 centred in NGC3351 obtained with the
Multi-Element Radio Linked Interferometer Network (MERLIN). We found 23
radio sources in this field, six of which are projected within the
D25 isophote of the galaxy and three are located inside the
central 100arcsec in radius. Two of these three are significantly
extended, while the third one is relatively compact. This one is the
only source with a previously detected counterpart at other wavelengths
and could constitute the radio counterpart of a young supernova remnant
(SNR). The other two are probably related to jets from a background
active galactic nucleus. We are not able to detect individual supernovae
(SNe) or SNRs in the central region (r < 600 pc) of the galaxy. This
could imply that the ionizing populations of the circumnuclear
star-forming regions are too young (less than a few Myr) to host SNe.
Also, the diffusion length of the relativistic electrons in the
interstellar medium associated with the SN from previous events of star
formation seems to be larger than our maximum resolution of 50 pc in
radius. Detecting the thermal bremsstrahlung emission from the
circumnuclear HII regions probably requires deeper observations.