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Recording description<\/h2>\n

Recorded with my Boren-Simon 10″ telescope and Apogee Ultra 8300 CCD with narrow band filters:<\/p>\n

Luminance #1: 20 minutes (Boren Simon, 10″ and\u00a0Apogee Ultra 8300 CCD)
\nLuminance #2: 30 minutes (T18, iTelescope.net)<\/p>\n

RGB: 10,10,10 minutes<\/p>\n

Processed with: MaximDL (stacking + DDP), PI (aligning and color combine), PS (features)<\/p>\n

 <\/p>\n

 <\/p>\n

 <\/p>\n

Object description<\/h2>\n

Maia Nebula \/\u00a0<\/em>NGC\u00a01432<\/em><\/b> is a\u00a0star<\/a>\u00a0in the\u00a0constellation<\/a>\u00a0of\u00a0Taurus<\/a>. It is the\u00a0fourth-brightest star<\/a>\u00a0in the\u00a0Pleiades<\/a>\u00a0open star cluster<\/a>\u00a0(M45<\/a>), after\u00a0Alcyone<\/a>,\u00a0Atlas<\/a>\u00a0and\u00a0Electra<\/a>, in that order. Maia is a\u00a0blue giant<\/a>of\u00a0spectral type<\/a>\u00a0B8 III, and a\u00a0mercury-manganese star<\/a>.<\/p>\n

Maia’s\u00a0visual magnitude<\/a>\u00a0is 3.871, requiring darker skies to be seen. Its total\u00a0bolometric<\/a>\u00a0luminosity<\/a>\u00a0is 660 times solar, mostly in the\u00a0ultraviolet<\/a>, thus suggesting a radius that is 5.5 times that of the Sun and a mass that is slightly more than 4 times solar.<\/sup>\u00a0It was thought to be a\u00a0variable star<\/a>\u00a0by astronomer\u00a0Otto Struve<\/a>. A class of stars known as\u00a0Maia variables<\/b>\u00a0was proposed, which included\u00a0Gamma Ursae Minoris<\/a>, but Maia and some others in the class have since been found to be stable.<\/sup><\/p>\n

Maia is one of the stars in the\u00a0Maia Nebula<\/b>\u00a0(also known as\u00a0NGC 1432<\/i>), a bright emission or reflection nebula<\/sup>\u00a0within the Pleiades star cluster.<\/p>\n

Source: Wikiepedia<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"

Recording description Recorded with my Boren-Simon 10″ telescope and Apogee Ultra 8300 CCD with narrow band filters: Luminance #1: 20 minutes (Boren Simon, 10″ and\u00a0Apogee Ultra 8300 CCD) Luminance #2: 30 minutes (T18, iTelescope.net) RGB: 10,10,10 minutes Processed with: MaximDL (stacking + DDP), PI (aligning and color combine), PS (features)       Object description […]<\/p>\n","protected":false},"author":1,"featured_media":2144,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"jetpack_post_was_ever_published":false,"jetpack_publicize_message":"","jetpack_is_tweetstorm":false,"jetpack_publicize_feature_enabled":true},"categories":[1],"tags":[],"jetpack_publicize_connections":[],"jetpack_featured_media_url":"https:\/\/i0.wp.com\/starworks.dk\/wp-content\/uploads\/2017\/11\/Maia-Nebula-LRGB_PI_PS_LessNoise.jpg?fit=2394%2C1880","jetpack_sharing_enabled":true,"jetpack_shortlink":"https:\/\/wp.me\/s6fUB9-ngc1432","jetpack_likes_enabled":true,"jetpack-related-posts":[{"id":2120,"url":"http:\/\/starworks.dk\/ngc4214\/","url_meta":{"origin":2143,"position":0},"title":"NGC4214","date":"01\/05\/2016","format":false,"excerpt":"Recording description Recorded with my Boren-Simon 10\" telescope and Apogee Ultra 8300 CCD with narrow band filters: Luminance: 65 minutes Ha: 75 minutes O3: 80 minuntes Processed in PixInsight and Photosop CS6. Blue channel is syntezised from luminance. \u00a0 \u00a0 Object description NGC 4214 is a dwarf barred irregular galaxy\u2026","rel":"","context":"In "Astronomy"","img":{"alt_text":"","src":"https:\/\/i0.wp.com\/starworks.dk\/wp-content\/uploads\/2016\/05\/NGC4214_ver2.jpg?fit=1200%2C893&resize=350%2C200","width":350,"height":200},"classes":[]}],"_links":{"self":[{"href":"http:\/\/starworks.dk\/wp-json\/wp\/v2\/posts\/2143"}],"collection":[{"href":"http:\/\/starworks.dk\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"http:\/\/starworks.dk\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"http:\/\/starworks.dk\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"http:\/\/starworks.dk\/wp-json\/wp\/v2\/comments?post=2143"}],"version-history":[{"count":2,"href":"http:\/\/starworks.dk\/wp-json\/wp\/v2\/posts\/2143\/revisions"}],"predecessor-version":[{"id":2221,"href":"http:\/\/starworks.dk\/wp-json\/wp\/v2\/posts\/2143\/revisions\/2221"}],"wp:featuredmedia":[{"embeddable":true,"href":"http:\/\/starworks.dk\/wp-json\/wp\/v2\/media\/2144"}],"wp:attachment":[{"href":"http:\/\/starworks.dk\/wp-json\/wp\/v2\/media?parent=2143"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"http:\/\/starworks.dk\/wp-json\/wp\/v2\/categories?post=2143"},{"taxonomy":"post_tag","embeddable":true,"href":"http:\/\/starworks.dk\/wp-json\/wp\/v2\/tags?post=2143"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}