{"id":7232,"date":"2025-04-21T14:58:12","date_gmt":"2025-04-21T05:58:12","guid":{"rendered":"https:\/\/www.astron.s.u-tokyo.ac.jp\/?page_id=7232"},"modified":"2026-03-23T15:20:28","modified_gmt":"2026-03-23T06:20:28","slug":"sanhueza_patricio","status":"publish","type":"page","link":"https:\/\/www.astron.s.u-tokyo.ac.jp\/en\/members\/doa\/sanhueza_patricio\/","title":{"rendered":"Patricio SANHUEZA"},"content":{"rendered":"<p><\/p>\n<h3>Patricio SANHUEZA<\/h3>\n<h4><span class=\"mw-headline\"> Research Field(s) <\/span><\/h4>\n<p>Radio Astronomy, Star Formation<\/p>\n<h4><span class=\"mw-headline\"> Research Subjects and Keywords <\/span><\/h4>\n<p>Early stages of high-mass star formation; Magnetic fields; Binary formation; Cloud fragmentation and chemistry; Infall streamers and accretion disks; Radio telescopes and interferometers<\/p>\n<h4><span class=\"mw-headline\"> Overview of Research <\/span><\/h4>\n<p>Using radio interferometers as primary tools, my research focuses on understanding the formation of high-mass stars. I am particularly interested in their earliest evolutionary stages, the role of magnetic fields, the formation of binary systems, the search for accretion disks and infall streamers, how the chemical composition help us to understand the physical processes, and also the origin of the initial mass function (IMF), among other key topics.<\/p>\n<h4><span class=\"mw-headline\"> Related Web Pages <\/span><\/h4>\n<p><a href=\"http:\/\/groups.astron.s.u-tokyo.ac.jp\/psanhueza\/index.html\" target=\"_blank\" rel=\"nofollow\">http:\/\/groups.astron.s.u-tokyo.ac.jp\/psanhueza\/index.html<\/a><\/p>\n<p><\/p>","protected":false},"excerpt":{"rendered":"<p>Patricio SANHUEZA Research Field(s) Radio Astronomy, Star Formation Research Subjects and Keywords Early stages of high-mass star formation; Magnetic fields; Binary formation; Cloud fragmentation and chemistry; Infall streamers and accretion disks; Radio telescopes and interferometers Overview of Research Using radio interferometers as primary tools, my research focuses on understanding the formation of high-mass stars. I <a class=\"read-more\" href=\"https:\/\/www.astron.s.u-tokyo.ac.jp\/en\/members\/doa\/sanhueza_patricio\/\">[ Read More ]<\/a><\/p>\n","protected":false},"author":22,"featured_media":0,"parent":172,"menu_order":12,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_monsterinsights_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"footnotes":""},"class_list":["post-7232","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/www.astron.s.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/pages\/7232","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.astron.s.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.astron.s.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.astron.s.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/users\/22"}],"replies":[{"embeddable":true,"href":"https:\/\/www.astron.s.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/comments?post=7232"}],"version-history":[{"count":18,"href":"https:\/\/www.astron.s.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/pages\/7232\/revisions"}],"predecessor-version":[{"id":7991,"href":"https:\/\/www.astron.s.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/pages\/7232\/revisions\/7991"}],"up":[{"embeddable":true,"href":"https:\/\/www.astron.s.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/pages\/172"}],"wp:attachment":[{"href":"https:\/\/www.astron.s.u-tokyo.ac.jp\/en\/wp-json\/wp\/v2\/media?parent=7232"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}