{"id":893,"date":"2018-02-22T15:35:28","date_gmt":"2018-02-22T15:35:28","guid":{"rendered":"http:\/\/grupodeespectroscopia.es\/MW\/?page_id=893"},"modified":"2025-05-14T21:56:25","modified_gmt":"2025-05-14T21:56:25","slug":"astrochemistry","status":"publish","type":"page","link":"https:\/\/grupodeespectroscopia.es\/MW\/astrochemistry\/","title":{"rendered":"Astrochemistry"},"content":{"rendered":"<p><a href=\"http:\/\/grupodeespectroscopia.es\/MW\/wp-content\/uploads\/2017\/10\/astrochemistry_MWregion.jpg\"><img decoding=\"async\" loading=\"lazy\" class=\"wp-image-851 tie-appear alignright\" src=\"http:\/\/grupodeespectroscopia.es\/MW\/wp-content\/uploads\/2017\/10\/astrochemistry_MWregion.jpg\" sizes=\"(max-width: 600px) 100vw, 600px\" srcset=\"http:\/\/grupodeespectroscopia.es\/MW\/wp-content\/uploads\/2017\/10\/astrochemistry_MWregion.jpg 1000w, http:\/\/grupodeespectroscopia.es\/MW\/wp-content\/uploads\/2017\/10\/astrochemistry_MWregion-300x206.jpg 300w, http:\/\/grupodeespectroscopia.es\/MW\/wp-content\/uploads\/2017\/10\/astrochemistry_MWregion-768x527.jpg 768w, http:\/\/grupodeespectroscopia.es\/MW\/wp-content\/uploads\/2017\/10\/astrochemistry_MWregion-110x75.jpg 110w\" alt=\"\" width=\"600\" height=\"412\" \/><\/a>The chemistry of the interstellar medium is uncertain, thus, our laboratory experiment are fundamental to guide the detection of different molecules in the space with the aim to improve the\u00a0 knowledge in this\u00a0 research field.<\/p>\n<p>The interstellar clouds are formed mostly by hydrogen but the presence of molecules such as halogenated compounds, hydrocarbons, and alcohols is proved .<\/p>\n<p>The interstellar clouds are important because from them, new stars are formed and consequently, new planets. For this reasons, the rotational spectra obtained in our laboratory, are necessary if we want to improve our chemical knowledge of the universe.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>The chemistry of the interstellar medium is uncertain, thus, our laboratory experiment are fundamental to guide the detection of different molecules in the space with the aim to improve the\u00a0 knowledge in this\u00a0 research field. The interstellar clouds are formed mostly by hydrogen but the presence of molecules such as halogenated compounds, hydrocarbons, and alcohols &hellip;<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":[],"acf":[],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/pages\/893"}],"collection":[{"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/comments?post=893"}],"version-history":[{"count":3,"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/pages\/893\/revisions"}],"predecessor-version":[{"id":1025,"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/pages\/893\/revisions\/1025"}],"wp:attachment":[{"href":"https:\/\/grupodeespectroscopia.es\/MW\/wp-json\/wp\/v2\/media?parent=893"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}