{"id":3593,"date":"2024-11-06T18:08:01","date_gmt":"2024-11-06T21:08:01","guid":{"rendered":"https:\/\/astro.uc.cl\/?post_type=charlas&p=3593"},"modified":"2024-11-20T12:50:38","modified_gmt":"2024-11-20T15:50:38","slug":"new-insights-into-the-dusty-hearts-of-local-ulirgs-yiqing-song","status":"publish","type":"charlas","link":"https:\/\/astro.uc.cl\/en\/charlas\/new-insights-into-the-dusty-hearts-of-local-ulirgs-yiqing-song\/","title":{"rendered":"New insights into the dusty hearts of local U\/LIRGs \u2013 Yiqing Song"},"content":{"rendered":"\n

Gas-rich galaxy mergers represent a crucial phase in the evolution of massive galaxies, where the host galaxy and the supermassive blackhole are thought to grow rapidly in tandem. Local IR-luminous galaxies provide the ideal laboratories to study in detail the extreme starburst and AGN activity triggered by such processes. However,\u00a0 heavy non-uniform dust extinction ubiquitously present in these systems makes this task challenging and necessitates a mulit-wavelength approach. In this talk, I will give an overview of recent efforts to characterize the nature of dust-obscured nuclei in local LIRGs and the associated feedback, in particular highlighting new results from high-resolution VLA and JWST studies from the Great Observatories All-sky LIRG Survey.\u00a0<\/p>\n\n\n\n

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