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- W3037817897 abstract "Luminous and Ultra-Luminous Infrared Galaxies (U/LIRGs) do also radiate copious amounts of radio emission, both thermal (free-free) and non-thermal (mainly synchrotron). This is very handy since, unlike optical and infra-red observations, radio is not obscured by the ubiquitous dust present in U/LIRGs, which allows a direct view of the ongoing activity in the hearts of those prolific star-forming galaxies. Here, I first justify the need for this high-angular resolution radio studies of local U/LIRGs, discuss the energy budget and the magnetic field, as well as IC and synchrotron losses in U/LIRGs, and present some selected results obtained by our team on high-angular resolution radio continuum studies of U/LIRGs. Among other results, I show the impressive discovery of an extremely prolific supernova factory in the central ~150 pc of the galaxy Arp 299-A (D=45 Mpc) and the monitoring of a large number of very compact radio sources in it, the detection and precise location of the long-sought AGN in Arp 299-A. A movie showing the appearance and disappearance of new SNe in Arp 299A can be found at this http URL All those results demonstrate that very-high angular resolution studies of nearby U/LIRGs are of high relevance for the comprehension of both local and high-z starbursting galaxies." @default.
- W3037817897 created "2020-07-02" @default.
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- W3037817897 date "2013-05-01" @default.
- W3037817897 modified "2023-10-16" @default.
- W3037817897 title "Digging deep into the ULIRG phenomenon: When radio beats dust" @default.
- W3037817897 hasPublicationYear "2013" @default.
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