{"id":5885,"date":"2015-08-24T15:59:37","date_gmt":"2015-08-24T15:59:37","guid":{"rendered":"http:\/\/revoscience.com\/en\/?p=5885"},"modified":"2015-08-24T15:59:37","modified_gmt":"2015-08-24T15:59:37","slug":"fierce-flashes-of-light-ripple","status":"publish","type":"post","link":"https:\/\/www.revoscience.com\/en\/fierce-flashes-of-light-ripple\/","title":{"rendered":"Fierce flashes of light ripple"},"content":{"rendered":"<figure id=\"attachment_5886\" aria-describedby=\"caption-attachment-5886\" style=\"width: 686px\" class=\"wp-caption alignright\"><a href=\"http:\/\/revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" decoding=\"async\" class=\"size-full wp-image-5886\" src=\"http:\/\/revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg\" alt=\"Feathery filaments in Mon R2 Credits: ESA\/Herschel\/PACS\/SPIRE\/HOBYS Key Programme consortium\" width=\"686\" height=\"700\" title=\"\" srcset=\"https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg 686w, https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2-294x300.jpg 294w\" sizes=\"auto, (max-width: 686px) 100vw, 686px\" \/><\/a><figcaption id=\"caption-attachment-5886\" class=\"wp-caption-text\">Feathery filaments in Mon R2 Credits: ESA\/Herschel\/PACS\/SPIRE\/HOBYS Key Programme consortium<\/figcaption><\/figure>\n<p style=\"color: #031e31; text-align: justify;\"><span style=\"color: #000000;\">Fierce flashes of light ripple through delicate tendrils of gas in this new image, from ESA\u2019s\u00a0<a style=\"color: #d0103a;\" href=\"http:\/\/www.esa.int\/Our_Activities\/Space_Science\/Herschel\" target=\"_blank\" rel=\"noopener\"><span style=\"color: #000000;\">Herschel<\/span><\/a>\u00a0space observatory, which shows the dramatic heart of a large and dense cosmic cloud known as Mon R2. This cloud lies some 2700 light-years away and is studded with hot, newly-formed stars.<\/span><\/p>\n<p style=\"color: #031e31; text-align: justify;\"><span style=\"color: #000000;\">[pullquote]Packed into the bright centre of this region are several hot \u2018bubbles\u2019 of ionised hydrogen, associated with newborn stars situated nearby[\/pullquote]. Here, gas heated to a temperature of 10 000 \u00b0C quickly expands outwards, inflating and enlarging over time. Herschel has explored the bubbles in Mon R2, finding them to have grown over the course of 100 000 to 350 000 years.<\/span><\/p>\n<p style=\"color: #031e31; text-align: justify;\"><span style=\"color: #000000;\">This process forms bubble-like cavities that lie within the larger Mon R2 cloud. These are known as HII regions and Mon R2 hosts four of them, clustered together in the central blue-white haze of bright light \u2014 one at the very centre, two stretching out like butterfly wings to the top left and bottom right, and another sitting just above the centre.<\/span><\/p>\n<p style=\"color: #031e31; text-align: justify;\"><span style=\"color: #000000;\">Each is associated with a different hot and luminous B-type star. These stars can be many times the mass of the Sun and usually appear with a blue hue due to their high temperature.<\/span><\/p>\n<p style=\"color: #031e31; text-align: justify;\"><span style=\"color: #000000;\">Astronomers have found that the hot bubbles in Mon R2 are enveloped by vast clouds of cold, dense gas, sitting within the filaments that stretch across the frame. In stark contrast to the gas in the hot bubbles, these clouds can be at temperatures as low as \u2013260 \u00b0C, just above absolute zero.<\/span><\/p>\n<p style=\"color: #031e31; text-align: justify;\"><span style=\"color: #000000;\">This\u00a0<a style=\"color: #d0103a;\" href=\"https:\/\/www.researchgate.net\/publication\/280307505_From_forced_collapse_to_H_ii_region_expansion_in_Mon_R2_Envelope_density_structure_and_age_determination_with_Herschel\" target=\"_blank\" rel=\"noopener\"><span style=\"color: #000000;\">particular cluster of HII regions<\/span><\/a>\u00a0has been studied as part of the Herschel imaging survey of OB young stellar objects, or\u00a0<a style=\"color: #d0103a;\" href=\"http:\/\/www.herschel.fr\/cea\/hobys\/en\/\" target=\"_blank\" rel=\"noopener\"><span style=\"color: #000000;\">HOBYS<\/span><\/a>, programme. This image combines multiple Herschel observations obtained with the PACS and SPIRE cameras and has been processed to highlight the cloud\u2019s clumpy complex of filaments, visible here in great and dramatic detail.<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Fierce flashes of light ripple through delicate tendrils of gas in this new image, from ESA\u2019s\u00a0Herschel\u00a0space observatory, which shows the dramatic heart of a large and dense cosmic cloud known as Mon R2. This cloud lies some 2700 light-years away and is studded with hot, newly-formed stars. [pullquote]Packed into the bright centre of this region [&hellip;]<\/p>\n","protected":false},"author":2,"featured_media":5886,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[42],"tags":[],"class_list":["post-5885","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-feature"],"featured_image_urls":{"full":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",686,700,false],"thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2-150x150.jpg",150,150,true],"medium":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2-294x300.jpg",294,300,true],"medium_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",686,700,false],"large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",686,700,false],"1536x1536":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",686,700,false],"2048x2048":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",686,700,false],"ultp_layout_landscape_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",686,700,false],"ultp_layout_landscape":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",559,570,false],"ultp_layout_portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",600,612,false],"ultp_layout_square":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",588,600,false],"newspaper-x-single-post":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",480,490,false],"newspaper-x-recent-post-big":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",353,360,false],"newspaper-x-recent-post-list-image":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",64,65,false],"web-stories-poster-portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",640,653,false],"web-stories-publisher-logo":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",94,96,false],"web-stories-thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2015\/08\/Feathery_filaments_in_Mon_R2_node_full_image_2.jpg",150,153,false]},"author_info":{"info":["RevoScience"]},"category_info":"<a href=\"https:\/\/www.revoscience.com\/en\/category\/feature\/\" rel=\"category tag\">Feature<\/a>","tag_info":"Feature","comment_count":"0","_links":{"self":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/5885","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/comments?post=5885"}],"version-history":[{"count":0,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/5885\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media\/5886"}],"wp:attachment":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media?parent=5885"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/categories?post=5885"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/tags?post=5885"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}