{"id":8238,"date":"2025-10-20T17:38:30","date_gmt":"2025-10-20T17:38:30","guid":{"rendered":"https:\/\/astronomia.udp.cl\/?post_type=event&#038;p=8238"},"modified":"2025-10-21T16:58:02","modified_gmt":"2025-10-21T16:58:02","slug":"the-muse-view-of-the-sculptor-galaxy","status":"publish","type":"event","link":"https:\/\/astronomia.udp.cl\/en\/event\/the-muse-view-of-the-sculptor-galaxy\/","title":{"rendered":"The MUSE view of the Sculptor galaxy"},"content":{"rendered":"\n<div class=\"wp-block-group is-nowrap is-layout-flex wp-container-1\">\n<h2 class=\"wp-block-heading has-medium-font-size\">Dr. Enrico Congiu, ESO<\/h2>\n\n\n\n<h2 class=\"wp-block-heading has-medium-font-size\">time TBD<\/h2>\n\n\n\n<h2 class=\"wp-block-heading has-medium-font-size\">FIC Auditorium<\/h2>\n<\/div>\n\n\n\n<div class=\"wp-block-media-text alignwide is-stacked-on-mobile\" style=\"grid-template-columns:19% auto\"><figure class=\"wp-block-media-text__media\"><img fetchpriority=\"high\" decoding=\"async\" width=\"830\" height=\"1024\" src=\"https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/10\/mugshot2-830x1024.jpg\" alt=\"\" class=\"wp-image-8240 size-full\" srcset=\"https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/10\/mugshot2-830x1024.jpg 830w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/10\/mugshot2-243x300.jpg 243w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/10\/mugshot2-768x947.jpg 768w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/10\/mugshot2-1245x1536.jpg 1245w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/10\/mugshot2-10x12.jpg 10w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/10\/mugshot2.jpg 1532w\" sizes=\"(max-width: 830px) 100vw, 830px\" \/><\/figure><div class=\"wp-block-media-text__content\">\n<p>High spatial resolution integral field observations of nearby galaxies revolutionized the field of galaxy evolution in the last decade. They allowed us to move from studying galaxies as single objects to investigating separtely the multitude of their building blocks (e.g., H II regions, molecular clouds, star clusters). However, most physical processes take place at small scales (~10 pc or less) that are difficult to resolve while keeping a complete view of the targeted system. In this context, we recently completed a 51 hours (20&#215;5 arcmin2) MUSE@VLT mosaic covering NGC 253, the Sculptor galaxy. With a distance of ~3.5 Mpc, NGC 253 is the closest massive starburst galaxy to the Milky Way and it offers us the possibility to study a wide variety of phenomena with a resolution of ~15 pc\/&#8221;, sufficient to resolve most of the ~5000 star-forming regions that are included in the mosaic (which extend up to 0.75* r_25). In this seminar, I will present the data and the preliminary results of the projects carried on by the PHANGS collaboration based on this dataset.<\/p>\n<\/div><\/div>\n","protected":false},"excerpt":{"rendered":"<p>UDP seminar by Dr. Enrico Congiu (ESO), time TBD<\/p>\n","protected":false},"featured_media":8244,"template":"","meta":{"_monsterinsights_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"site-sidebar-layout":"default","site-content-layout":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"","ast-breadcrumbs-content":"","ast-featured-img":"disabled","footer-sml-layout":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":""},"event-category":[263],"acf":[],"_links":{"self":[{"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/event\/8238"}],"collection":[{"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/event"}],"about":[{"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/types\/event"}],"version-history":[{"count":5,"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/event\/8238\/revisions"}],"predecessor-version":[{"id":8250,"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/event\/8238\/revisions\/8250"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/media\/8244"}],"wp:attachment":[{"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/media?parent=8238"}],"wp:term":[{"taxonomy":"event-category","embeddable":true,"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/event-category?post=8238"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}