TY  - GEN 
AU  - Leon, S.
AU  - Verdes-Montenegro, L.
AU  - Sabater, J.
AU  - Espada Fernández, Daniel
AU  - Lisenfeld , Ute
AU  - Ballu, A.
AU  - Sulentic, J.
AU  - Verley, Simon
AU  - Bergond, G.
AU  - García, E.
PY  - 2008
SN  - 0004-6361
SN  - 1432-0746
UR  - http://hdl.handle.net/10481/28396
AB  - Context. This paper is part of a series that describes the results of the AMIGA (Analysis of the interstellar Medium of Isolated GAlaxies) project, studying the largest sample of very isolated galaxies in the local Universe.
AB  - Aims. The study of the radio properties of the AMIGA sample is intended to characterize the radio continuum emission for a sample least affected by the local environment, thus providing a reference against which less isolated and interacting samples...
AB  - Results. A catalog of radio fluxes was obtained from the above four surveys. Comparison between the NVSS and FIRST detections indicates that the radio continuum is coming from disk-dominated emission in spiral galaxies, in contrast to the results...
AB  - Conclusions. The results indicate the very low level of radio continuum emission in our sample of isolated galaxies, which is dominated by mild disk SF. It confirms thus the AMIGA sample as a suitable template to effectively quantify the role of...
LA  - eng
PB  - European Southern Observatory (ESO); Springer Verlag
KW  - Galaxies
KW  - Evolution
KW  - Luminosity function
KW  - Radio continuum
KW  - Surveys
KW  - Mass function
TI  - The AMIGA sample of isolated galaxies: VI Radio continuum properties of isolated galaxies: a very radio quiet sample
DO  - 10.1051/0004-6361:20078533
ER  -