Wojciech S. Jurusik, Krzysztof T. Chyzy, Robert T. Drzazga
Published 2013-05-29Version 1
The radio emission of normal galaxies may become opaque at low radio frequencies due to thermal ionized gas. We performed modelling of the free-free absorption to reproduce the ocal spectrum of SgrA Complex and the global spectrum of the starburst galaxy M82. We show the importance of resolution of radio observations and the value of filling factor of the absorbing gas for correct modelling of the absorption.
Comments: proceedings of the conference: Magnetic Fields in the Universe: From Laboratory and Stars to Primordial Structures Aug. 21st - 27th 2011, Zakopane, Poland, Eds. M. Soida, K. Otmianowska-Mazur, E.M. de Gouveia Dal Pino & A. Lazarian
Multi-messenger model for the starburst galaxy M82
Luminosity Evolution of the Hot Gas in Normal Galaxies from the Near Universe to z=0.5
High-resolution radio study of SNR IC443 at low radio frequencies
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