{"id":56,"date":"2017-02-01T09:42:27","date_gmt":"2017-02-01T09:42:27","guid":{"rendered":"http:\/\/sites.dev.dundee.ac.uk\/asiciliaaguilar\/?page_id=56"},"modified":"2021-05-03T09:37:13","modified_gmt":"2021-05-03T08:37:13","slug":"a-multiwavelength-journey-through-tr-37","status":"publish","type":"page","link":"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/a-multiwavelength-journey-through-tr-37\/","title":{"rendered":"A Multiwavelength Journey through Tr 37"},"content":{"rendered":"<p style=\"text-align: justify\">Tr 37 is a young star-forming region located at the edge of the Cep OB2 bubble, centered at the O6 star HD 206267. The main population around HD 206267 has typical ages of 4 Myr. The O6 star illuminates a bright globule to the west of the cluster, where younger stars are found.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"alignnone wp-image-19 size-large\" src=\"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/wavelength_journey-1024x768.jpg\" alt=\"wavelength_journey\" width=\"660\" height=\"495\" srcset=\"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/wavelength_journey-1024x768.jpg 1024w, https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/wavelength_journey-300x225.jpg 300w, https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/wavelength_journey-768x576.jpg 768w, https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/wavelength_journey-624x468.jpg 624w\" sizes=\"auto, (max-width: 660px) 100vw, 660px\" \/><\/p>\n<p style=\"text-align: justify\">But the story does not end here: Herschel shows the very hidden population that had even escaped the eyes of Spitzer, a new star born at the tip of the globule. Have a look at it at Herschel\/PACS wavelengths (70 and 160 microns, left and right respectively):<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"alignnone wp-image-21\" src=\"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/globule_mosaic_70um_160um-300x115.jpg\" alt=\"globule_mosaic_70um_160um\" width=\"783\" height=\"300\" srcset=\"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/globule_mosaic_70um_160um-300x115.jpg 300w, https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/globule_mosaic_70um_160um-768x294.jpg 768w, https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/globule_mosaic_70um_160um-1024x392.jpg 1024w, https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/globule_mosaic_70um_160um-624x239.jpg 624w\" sizes=\"auto, (max-width: 783px) 100vw, 783px\" \/><\/p>\n<p>And zooming in around the new object:<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" class=\"alignnone wp-image-22\" src=\"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/newsource_70_160-300x118.jpg\" alt=\"newsource_70_160\" width=\"764\" height=\"300\" srcset=\"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/newsource_70_160-300x118.jpg 300w, https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/newsource_70_160-768x302.jpg 768w, https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/newsource_70_160-1024x402.jpg 1024w, https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-content\/uploads\/sites\/71\/2017\/01\/newsource_70_160-624x245.jpg 624w\" sizes=\"auto, (max-width: 764px) 100vw, 764px\" \/><\/p>\n<p>Learn more <strong><a href=\"http:\/\/arxiv.org\/abs\/1312.3867\"> here<\/a><\/strong>.<\/p>\n<p>Or check some popular papers (in Spanish):<\/p>\n<p><strong><a href=\"https:\/\/www.uam.es\/ss\/Satellite\/es\/1242652961025\/1242669371963\/articulo\/articulo\/Erupciones_en_la_estrella_EX_Lupi:_experimentos_estelares_en_tiempo_real.htm\"> Erupciones en la estrella EX Lupi: Experimentos estelares en tiempo real<\/a><\/strong><\/p>\n<p><strong><a href=\"http:\/\/www.uam.es\/ss\/Satellite\/es\/1242652962164\/1242661952463\/notcientifica\/notCientific\/%3FComo_era_nuestro_Sistema_Solar_en_sus_comienzos%3F.htm\"> \u00bfC\u00f3mo era nuestro Sistema Solar en sus comienzos? <\/a><\/strong><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tr 37 is a young star-forming region located at the edge of the Cep OB2 bubble, centered at the O6 star HD 206267. The main population around HD 206267 has typical ages of 4 Myr. The O6 star illuminates a bright globule to the west of the cluster, where younger stars are found. But the [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-56","page","type-page","status-publish","hentry"],"blocksy_meta":[],"_links":{"self":[{"href":"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-json\/wp\/v2\/pages\/56","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-json\/wp\/v2\/comments?post=56"}],"version-history":[{"count":1,"href":"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-json\/wp\/v2\/pages\/56\/revisions"}],"predecessor-version":[{"id":363,"href":"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-json\/wp\/v2\/pages\/56\/revisions\/363"}],"wp:attachment":[{"href":"https:\/\/sites.dundee.ac.uk\/asiciliaaguilar\/wp-json\/wp\/v2\/media?parent=56"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}