{"id":2034,"date":"2020-01-20T15:21:37","date_gmt":"2020-01-20T14:21:37","guid":{"rendered":"http:\/\/www.vulkanlandsternwarte.at\/?p=2034"},"modified":"2021-09-30T16:51:38","modified_gmt":"2021-09-30T14:51:38","slug":"flaming-star-nebula-in-haoii-rgb","status":"publish","type":"post","link":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wordpress\/2020\/01\/20\/flaming-star-nebula-in-haoii-rgb\/","title":{"rendered":"&#8222;Flaming Star Nebula&#8220;"},"content":{"rendered":"<p>Dieser Gasnebel im Sternbild Fuhrmann ist ein Mix aus&nbsp; Reflexions- und Emissionsnebel.&nbsp; Der namensgebende Stern ionisiert mit seiner Strahlung&nbsp;das Wasserstoffgas. Bei der Rekombination der Elektronen entsteht das charakteristische rote Leuchten bei 656nm Wellenl\u00e4nge.<\/p>\n<figure id=\"attachment_2035\" aria-describedby=\"caption-attachment-2035\" style=\"width: 525px\" class=\"wp-caption alignnone\"><a href=\"https:\/\/www.vulkanlandsternwarte.at\/wordpress\/wp-content\/uploads\/2020\/01\/FlamingStarNebula.jpg\"><img loading=\"lazy\" decoding=\"async\" class=\"size-large wp-image-2035\" src=\"https:\/\/www.vulkanlandsternwarte.at\/wordpress\/wp-content\/uploads\/2020\/01\/FlamingStarNebula-683x1024.jpg\" alt=\"\" width=\"525\" height=\"787\" srcset=\"https:\/\/www.vulkanlandsternwarte.at\/wordpress\/wp-content\/uploads\/2020\/01\/FlamingStarNebula-683x1024.jpg 683w, https:\/\/www.vulkanlandsternwarte.at\/wordpress\/wp-content\/uploads\/2020\/01\/FlamingStarNebula-200x300.jpg 200w, https:\/\/www.vulkanlandsternwarte.at\/wordpress\/wp-content\/uploads\/2020\/01\/FlamingStarNebula-768x1151.jpg 768w, https:\/\/www.vulkanlandsternwarte.at\/wordpress\/wp-content\/uploads\/2020\/01\/FlamingStarNebula.jpg 934w\" sizes=\"auto, (max-width: 525px) 100vw, 525px\" \/><\/a><figcaption id=\"caption-attachment-2035\" class=\"wp-caption-text\">10 Zoll Newton + NIKON DSLR<\/figcaption><\/figure>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Dieser Gasnebel im Sternbild Fuhrmann ist ein Mix aus&nbsp; Reflexions- und Emissionsnebel.&nbsp; Der namensgebende Stern ionisiert mit seiner Strahlung&nbsp;das Wasserstoffgas. Bei der Rekombination der Elektronen entsteht das charakteristische rote Leuchten bei 656nm Wellenl\u00e4nge. &nbsp;<\/p>\n","protected":false},"author":9,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"image","meta":{"footnotes":""},"categories":[21],"tags":[],"class_list":["post-2034","post","type-post","status-publish","format-image","hentry","category-astrophotographie","post_format-post-format-image"],"_links":{"self":[{"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/posts\/2034","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/users\/9"}],"replies":[{"embeddable":true,"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/comments?post=2034"}],"version-history":[{"count":4,"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/posts\/2034\/revisions"}],"predecessor-version":[{"id":3579,"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/posts\/2034\/revisions\/3579"}],"wp:attachment":[{"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/media?parent=2034"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/categories?post=2034"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.vulkanlandsternwarte.at\/index.php\/wp-json\/wp\/v2\/tags?post=2034"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}