2001/03/09 by A. Bressan, Bressan, A., G. L. Granato +3
Engineering · Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Galaxies: Formation, Evolution, Phenomena #Semiconductor Lasers and Optical Devices #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0103148
3 pages; poster presented at the Workshop on "QSO Hosts And Their Environments", 10-12 Jan 2001, Granada, Spain
arxiv created 2001/03/09 · openalex publication_date 2001/03/09 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We examine the tight correlation observed between the far infrared (FIR) and radio emission in normal and star burst galaxies. We show that significant deviations from the average relation are to be expected in young star burst or post star burst galaxies, due to the different fading times of FIR and Radio power.