On its surface, it appears to be another 2D pixelated action game. It’s a new year and another opportunity for indie developers to flex their roguelike creativity. Review code provided with many thanks to Stride Pr 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.Developer|Publisher: Molton Studio| Raiser Games A movie showing the appearance and disappearance of new SNe in Arp 299A can be found at this http URL. 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. 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. 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. Perez-Torres Download PDF 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). Download a PDF of the paper titled Digging deep into the ULIRG phenomenon: When radio beats dust, by Miguel A.
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