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- W6318119 abstract "I review some of the main results obtained by our team in the last few years on high-angular resolution radio studies of nearby Luminous and Ultra-Luminous Infrared Galaxies (LIRGs and ULIRGs, respectively). These galaxies are expected to form stars at rates (gtrsim )(10–100) (mathrm{M}_{odot },mathrm{{year}}^{-1}), and produce core-collapse supernovae at rates (gtrsim )(0.3–3) year− 1. (U)LIRGs are also expected to be bright at radio wavelengths, thanks to the ubiquitous Far-Infrared Radio correlation, which makes high-angular resolution ((lesssim 0.1^{primeprime})) radio observations an excellent tool for probing the inner ≃ 100 pc region of local (U)LIRGs. I justify the need for this high-angular resolution radio studies of local (U)LIRGs and, among other results, I present 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 and, more recently, the evidence for the existence of nuclear disks ((lesssim )100 pc in size) in starburst galaxies from their radial distribution of supernovae. All those results show 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.
- W6318119 created "2016-06-24" @default.
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- W6318119 date "2013-01-01" @default.
- W6318119 modified "2023-09-25" @default.
- W6318119 title "The Central Regions of Local (U)LIRGs Viewed with Big Radio Eyes" @default.
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- W6318119 doi "https://doi.org/10.1007/978-3-642-35410-6_11" @default.
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