{"id":6904,"date":"2025-07-18T23:24:07","date_gmt":"2025-07-18T23:24:07","guid":{"rendered":"https:\/\/astronomia.udp.cl\/?post_type=area&#038;p=6904"},"modified":"2025-08-28T16:44:18","modified_gmt":"2025-08-28T16:44:18","slug":"stellar-and-galactic-astronomy","status":"publish","type":"area","link":"https:\/\/astronomia.udp.cl\/en\/area\/stellar-and-galactic-astronomy\/","title":{"rendered":"Stellar and Galactic Astronomy"},"content":{"rendered":"\t\t<div data-elementor-type=\"wp-post\" data-elementor-id=\"6904\" class=\"elementor elementor-6904\" data-elementor-settings=\"{&quot;ha_cmc_init_switcher&quot;:&quot;no&quot;}\">\n\t\t\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-b3f364f elementor-section-height-min-height elementor-section-boxed elementor-section-height-default elementor-section-items-middle\" data-id=\"b3f364f\" data-element_type=\"section\" data-settings=\"{&quot;background_background&quot;:&quot;classic&quot;,&quot;_ha_eqh_enable&quot;:false}\">\n\t\t\t\t\t\t\t<div class=\"elementor-background-overlay\"><\/div>\n\t\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-no\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-1105de6\" data-id=\"1105de6\" data-element_type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-a81c241 elementor-widget elementor-widget-heading\" data-id=\"a81c241\" data-element_type=\"widget\" data-widget_type=\"heading.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t<style>\/*! elementor - v3.20.0 - 13-03-2024 *\/\n.elementor-heading-title{padding:0;margin:0;line-height:1}.elementor-widget-heading .elementor-heading-title[class*=elementor-size-]>a{color:inherit;font-size:inherit;line-height:inherit}.elementor-widget-heading .elementor-heading-title.elementor-size-small{font-size:15px}.elementor-widget-heading .elementor-heading-title.elementor-size-medium{font-size:19px}.elementor-widget-heading .elementor-heading-title.elementor-size-large{font-size:29px}.elementor-widget-heading .elementor-heading-title.elementor-size-xl{font-size:39px}.elementor-widget-heading .elementor-heading-title.elementor-size-xxl{font-size:59px}<\/style><h1 class=\"elementor-heading-title elementor-size-default\">Stellar and Galactic Astronomy<\/h1>\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-0c8dddc elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"0c8dddc\" data-element_type=\"section\" data-settings=\"{&quot;_ha_eqh_enable&quot;:false}\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-86f0afe\" data-id=\"86f0afe\" data-element_type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-d5eaa6b animated-slow elementor-invisible elementor-widget elementor-widget-heading\" data-id=\"d5eaa6b\" data-element_type=\"widget\" data-settings=\"{&quot;_animation&quot;:&quot;fadeIn&quot;,&quot;_animation_delay&quot;:700}\" data-widget_type=\"heading.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t<h5 class=\"elementor-heading-title elementor-size-default\">Stars are the candles of the Universe, and as such the Stellar and Galactic Astronomy area is the window through which we study their structure and life cycle to answer an extensive variety of astrophysical phenomena. At the IEA, we study the stars as <i>complex celestial objects,<\/i> stars as <i>explosive and variable objects<\/i>, stars as <i>key components of galaxies<\/i>, and stars as <i>planet hosts<\/i>.  Explore below featured projects in each section.<\/h5>\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-3538734 elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"3538734\" data-element_type=\"section\" data-settings=\"{&quot;_ha_eqh_enable&quot;:false}\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-4a45ac7\" data-id=\"4a45ac7\" data-element_type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-ccee0b6 animated-slow elementor-invisible elementor-widget elementor-widget-text-editor\" data-id=\"ccee0b6\" data-element_type=\"widget\" data-settings=\"{&quot;_animation&quot;:&quot;fadeIn&quot;,&quot;_animation_delay&quot;:700}\" data-widget_type=\"text-editor.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t<style>\/*! elementor - v3.20.0 - 13-03-2024 *\/\n.elementor-widget-text-editor.elementor-drop-cap-view-stacked .elementor-drop-cap{background-color:#69727d;color:#fff}.elementor-widget-text-editor.elementor-drop-cap-view-framed .elementor-drop-cap{color:#69727d;border:3px solid;background-color:transparent}.elementor-widget-text-editor:not(.elementor-drop-cap-view-default) .elementor-drop-cap{margin-top:8px}.elementor-widget-text-editor:not(.elementor-drop-cap-view-default) .elementor-drop-cap-letter{width:1em;height:1em}.elementor-widget-text-editor .elementor-drop-cap{float:left;text-align:center;line-height:1;font-size:50px}.elementor-widget-text-editor .elementor-drop-cap-letter{display:inline-block}<\/style>\t\t\t\t<p>This area focuses on the study of stars and stellar phenomena for a variety of applications. Among these, we emphasize stellar spectroscopy, transients, supernova events and stellar populations in the Milky Way and near-by galaxies.<\/p><p>We are heavily involved in projects such as ASAS-SN to detect and study various explosive transient events in the Universe and also variable stars in the Milky Way and local galaxies. Supernovae are of great interest not only because they mark the deaths of stars, but also because they contribute to the chemical enrichment of the Universe, can be used to estimate precise distances to galaxies,&nbsp; and they interact with their surroundings, influencing the evolution of galaxies. We use optical and near-IR observations (photometry and spectroscopy) from different telescopes to study the properties of explosive transient events and their host galaxy environments to study their progenitor stars and explosion physics.<\/p><p>Our research also focuses on stellar atmospheres, particularly the determination of stellar parameters and chemical abundances for thousands of stars. This information is then used to analyze the stellar populations of the Milky Way and neighboring galaxies, allowing us to reconstruct the formation and evolution of spiral galaxies by using their chemical compositions as fossil records.<\/p><p>Thanks to SDSS-V\u2014specifically the combination of the Milky Way Mapper and the Local Volume Mapper\u2014new opportunities are emerging to integrate stellar spectra with the chemical properties of the interstellar medium (ISM) in the Milky Way. This will revolutionize our understanding of how galaxies like our own assemble. Our expertise in analyzing both high-resolution stellar spectra (e.g., from MIKE, UVES, APOGEE) and high-quality integral field unit (IFU) data (e.g., from MUSE) has led us to play a leading role in key working groups within both the Milky Way Mapper and the Local Volume Mapper.<br>Other topics of interest in this area include compact objects, binary stars, variable stars, dwarf galaxies, metal-poor stars and planet-host stars.<\/p>\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-a7225e9 elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"a7225e9\" data-element_type=\"section\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-2653ec3\" data-id=\"2653ec3\" data-element_type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-6f3ffbd ha-card--left ha-card--tablet-top ha-card--mobile-top ha-has-bg-overlay elementor-widget elementor-widget-ha-card happy-addon ha-card\" data-id=\"6f3ffbd\" data-element_type=\"widget\" data-widget_type=\"ha-card.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\n\t\t\t\t\t<figure class=\"ha-card-figure\">\n\t\t\t\t<img fetchpriority=\"high\" width=\"1280\" height=\"1275\" src=\"https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/hr-diagram.jpg\" class=\"attachment-full size-full wp-image-6937\" alt=\"\" decoding=\"async\" srcset=\"https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/hr-diagram.jpg 1280w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/hr-diagram-300x300.jpg 300w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/hr-diagram-1024x1020.jpg 1024w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/hr-diagram-150x150.jpg 150w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/hr-diagram-768x765.jpg 768w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/hr-diagram-12x12.jpg 12w\" sizes=\"(max-width: 1280px) 100vw, 1280px\" \/>\t\t\t\t\t\t\t<\/figure>\n\t\t\n\t\t<div class=\"ha-card-body\">\n\n\t\t\t<h3 class=\"ha-card-title\">Stellar Structure and Evolution<\/h3>\n\t\t\t\t\t\t\t<div class=\"ha-card-text\">\n\t\t\t\t\t<p>From massive stars to cool dwarfs, we study the physical processes behind how stars are born, evolve, and how they are affected by internal and environmental factors. By modeling stellar atmospheres, binary interactions, and investigating fundamental parameters across the evolutionary phases in the HR diagram, we try to understand the physical mechanisms that govern the life-cycle of stars in our Galaxy and beyond.<\/p>\n\t\t\t\t<\/div>\n\t\t\t\n\t\t\t\t\t\t\t<a class=\"ha-btn ha-btn--icon-before\" href=\"https:\/\/astronomia.udp.cl\/research\/areas\/stellar-structure\/\" target=\"_blank\"><i class=\"ha-btn-icon fas fa-star\" aria-hidden=\"true\"><\/i> <span class=\"ha-btn-text\">Explore featured projects<\/span><\/a>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-6a70ce5 elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"6a70ce5\" data-element_type=\"section\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-c2034a2\" data-id=\"c2034a2\" data-element_type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-bea1a62 ha-card--right ha-card--tablet-top ha-card--mobile-top ha-has-bg-overlay elementor-widget elementor-widget-ha-card happy-addon ha-card\" data-id=\"bea1a62\" data-element_type=\"widget\" data-widget_type=\"ha-card.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\n\t\t\t\t\t<figure class=\"ha-card-figure\">\n\t\t\t\t<img width=\"926\" height=\"920\" src=\"https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/SN-image.png\" class=\"attachment-full size-full wp-image-6936\" alt=\"\" decoding=\"async\" srcset=\"https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/SN-image.png 926w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/SN-image-300x298.png 300w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/SN-image-150x150.png 150w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/SN-image-768x763.png 768w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/SN-image-12x12.png 12w\" sizes=\"(max-width: 926px) 100vw, 926px\" \/>\t\t\t\t\t\t\t<\/figure>\n\t\t\n\t\t<div class=\"ha-card-body\">\n\n\t\t\t<h3 class=\"ha-card-title\">Supernovae, Transients, and Variable Stars<\/h3>\n\t\t\t\t\t\t\t<div class=\"ha-card-text\">\n\t\t\t\t\t<p>We explore the dramatic explosive stages that mark the deaths of stars \u2014 supernovae \u2014 to unveil the nature of their progenitors. Our research also focusses on the physics driving transient phenomena and variable stars, and the impact they have on galaxy environments through feedback. Through time-domain surveys and targeted follow-up, our work allows us to trace how transient events shape galaxy evolution.<\/p>\n\t\t\t\t<\/div>\n\t\t\t\n\t\t\t\t\t\t\t<a class=\"ha-btn ha-btn--icon-before\" href=\"https:\/\/astronomia.udp.cl\/research\/areas\/transients\/\" target=\"_blank\"><i class=\"ha-btn-icon fas fa-star\" aria-hidden=\"true\"><\/i> <span class=\"ha-btn-text\">Explore featured projects<\/span><\/a>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-f5d9d02 elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"f5d9d02\" data-element_type=\"section\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-007389d\" data-id=\"007389d\" data-element_type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-44880d6 ha-card--left ha-card--tablet-top ha-card--mobile-top ha-has-bg-overlay elementor-widget elementor-widget-ha-card happy-addon ha-card\" data-id=\"44880d6\" data-element_type=\"widget\" data-widget_type=\"ha-card.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\n\t\t\t\t\t<figure class=\"ha-card-figure\">\n\t\t\t\t<img width=\"860\" height=\"860\" src=\"https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/stellar-pops.webp\" class=\"attachment-full size-full wp-image-6929\" alt=\"\" decoding=\"async\" srcset=\"https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/stellar-pops.webp 860w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/stellar-pops-300x300.webp 300w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/stellar-pops-150x150.webp 150w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/stellar-pops-768x768.webp 768w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/stellar-pops-12x12.webp 12w\" sizes=\"(max-width: 860px) 100vw, 860px\" \/>\t\t\t\t\t\t\t<\/figure>\n\t\t\n\t\t<div class=\"ha-card-body\">\n\n\t\t\t<h3 class=\"ha-card-title\">Stellar populations<\/h3>\n\t\t\t\t\t\t\t<div class=\"ha-card-text\">\n\t\t\t\t\t<p>To uncover the assembly history of the Milky Way and its neighbors, we decode the fossil records preserved in their stellar populations through Galactic Archaeology. Our work involves chemical tagging, kinematics analyses, and tracing star formation histories, and galactic phylogenetics using simulations and large spectroscopic surveys like the Milky Way Mapper and the Local Volume Mapper. With these instruments and techniques, we trace galaxy evolution across the Local Universe.<\/p>\n\t\t\t\t<\/div>\n\t\t\t\n\t\t\t\t\t\t\t<a class=\"ha-btn ha-btn--icon-before\" href=\"https:\/\/astronomia.udp.cl\/research\/areas\/stellar-populations\/\" target=\"_blank\"><i class=\"ha-btn-icon fas fa-star\" aria-hidden=\"true\"><\/i> <span class=\"ha-btn-text\">Explore featured projects<\/span><\/a>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<section class=\"elementor-section elementor-top-section elementor-element elementor-element-2d6350f elementor-section-boxed elementor-section-height-default elementor-section-height-default\" data-id=\"2d6350f\" data-element_type=\"section\">\n\t\t\t\t\t\t<div class=\"elementor-container elementor-column-gap-default\">\n\t\t\t\t\t<div class=\"elementor-column elementor-col-100 elementor-top-column elementor-element elementor-element-7adce35\" data-id=\"7adce35\" data-element_type=\"column\">\n\t\t\t<div class=\"elementor-widget-wrap elementor-element-populated\">\n\t\t\t\t\t\t<div class=\"elementor-element elementor-element-d629270 ha-card--right ha-card--tablet-top ha-card--mobile-top ha-has-bg-overlay elementor-widget elementor-widget-ha-card happy-addon ha-card\" data-id=\"d629270\" data-element_type=\"widget\" data-widget_type=\"ha-card.default\">\n\t\t\t\t<div class=\"elementor-widget-container\">\n\t\t\t\n\t\t\t\t\t<figure class=\"ha-card-figure\">\n\t\t\t\t<img loading=\"lazy\" width=\"2560\" height=\"2048\" src=\"https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/polluted-white-dwarf-scaled.jpeg\" class=\"attachment-full size-full wp-image-7030\" alt=\"\" decoding=\"async\" srcset=\"https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/polluted-white-dwarf-scaled.jpeg 2560w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/polluted-white-dwarf-300x240.jpeg 300w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/polluted-white-dwarf-1024x819.jpeg 1024w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/polluted-white-dwarf-768x614.jpeg 768w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/polluted-white-dwarf-1536x1229.jpeg 1536w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/polluted-white-dwarf-2048x1638.jpeg 2048w, https:\/\/astronomia.udp.cl\/wp-content\/uploads\/2025\/07\/polluted-white-dwarf-15x12.jpeg 15w\" sizes=\"(max-width: 2560px) 100vw, 2560px\" \/>\t\t\t\t\t\t\t<\/figure>\n\t\t\n\t\t<div class=\"ha-card-body\">\n\n\t\t\t<h3 class=\"ha-card-title\">Stars as Planet Hosts<\/h3>\n\t\t\t\t\t\t\t<div class=\"ha-card-text\">\n\t\t\t\t\t<p>Stars often host planetary systems that form from the same molecular cloud. Studying stars and the material they accrete allows us to probe the formation, evolution, and composition of their planetary companions. By combining stellar and planetary chemistry, we study the building blocks and the physical processes that govern planet formation around stellar hosts.<\/p>\n\t\t\t\t<\/div>\n\t\t\t\n\t\t\t\t\t\t\t<a class=\"ha-btn ha-btn--icon-before\" href=\"https:\/\/astronomia.udp.cl\/research\/areas\/stars-as-planet-hosts\/\" target=\"_blank\"><i class=\"ha-btn-icon fas fa-star\" aria-hidden=\"true\"><\/i> <span class=\"ha-btn-text\">Explore featured projects<\/span><\/a>\n\t\t\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/div>\n\t\t\t\t\t<\/div>\n\t\t<\/section>\n\t\t\t\t<\/div>\n\t\t","protected":false},"featured_media":6452,"template":"","meta":{"_monsterinsights_skip_tracking":false,"_monsterinsights_sitenote_active":false,"_monsterinsights_sitenote_note":"","_monsterinsights_sitenote_category":0,"site-sidebar-layout":"no-sidebar","site-content-layout":"page-builder","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":"disabled","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":""},"acf":[],"_links":{"self":[{"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/area\/6904"}],"collection":[{"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/area"}],"about":[{"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/types\/area"}],"version-history":[{"count":37,"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/area\/6904\/revisions"}],"predecessor-version":[{"id":8125,"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/area\/6904\/revisions\/8125"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/media\/6452"}],"wp:attachment":[{"href":"https:\/\/astronomia.udp.cl\/en\/wp-json\/wp\/v2\/media?parent=6904"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}