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2011. 12 123. 1 805. -2 718. 211 772. 704.

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Cederblad 214 is the brightest part of the NGC 7822 complex, strangely enough PixInsights’ annotation script regards this one alone as NGC 7822, which IMO also includes the loop from the previous post.See Astrobin for more details. A Cederblad 214 egy hatalmas kiterjedésű emissziós ködösség a Cepheus csillagképben, pontosabban a Cepheus és a Cassiopeia határvidékén. Maga a ködösség rendkívül nehezen észlelhető vizuálisan. Fotografikus úton könnyebb megörökíteni, de igazán csak a speciális keskenysávú szűrőkkel lehet a mély részleteit bemutatni.

We mainly image Deep Sky Objects, indulge in Lunar Photography Kontakta Jakob Cederblad, 30 år, Malmö. Adress: Vitemöllegatan 5, Postnummer: 214 42 - Hitta mer här! Oct 26, 2014 Sharpless 171 incorporates NGC 7822 and the active region Cederblad 214, much of which is imaged above.

Jakob Sebastian Cederblad Malmö, 30 år - Merinfo.se

Subscribe to the ESA/Hubble Media Newsletter. Cederblad 214 is one of the hottest known stars in our stellar neighborhood. With a temperature of almost 45,000 degrees Kelvin, BD+66 1673 is over 100,000 times more luminous than our own Sun. Acquisition details: Ha 175 x 150s SII 225 x 150s OIII 200 x 150s Total 25hours integration time ASI183MM RASA 8" CEM120. See More.

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Cederblad 214 by Yves, on Flickr Cederblad 214 / NGC7822 / Frågeteckennebulosan. Tillagt av Per Johansson den 25 December 2020 kl. 18.05; Se Bilder; Föregående | Nästa; Mitt rekord i exptid tror About this Object: The young stellar association Cepheus OB4 lies in a region of bright nebulosity known as NGC 7822 and S 171. The fainter northern arch of nebulosity is designated NGC 7822(North up East left) and the brighter southern cloud is designated S 171 (Sharpless, 1959) or alternatively Cederblad 214. Query : Cederblad 214 C.D.S.

The fainter northern arch of nebulosity is designated NGC 7822(North up East left) and the brighter southern cloud is designated S 171 (Sharpless, 1959) or alternatively Cederblad 214. Cederblad 214. Located in the constellation Cepheus 214 is part of a huge emission nebula. Like many nebula of this type it is a very active star nursery.
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View profile Send private message Remove shadow-ban Share; Navigation context User gallery All image uploads Cederblad 214, NGC7822 - SHO - 2x2 mosaic. Technical card Imaging telescopes or lenses: Astro-Physics 92mm f/6.65 Stowaway · Astro-Physics 152mm f/7.5 Starfire EDF Imaging cameras: ZWO ASI2600MC-Pro ASI2600MC Cederblad 214 Part of NGC 7822 – Oct 2018 – Bicolor v1. Yet another bicolor processing of old data from 2018. Cederblad 214 is the brightest part of the NGC 7822 complex, strangely enough PixInsights’ annotation script regards this one alone as NGC 7822, which IMO also includes the loop from the previous post.See Astrobin for more details.

top (suggested) NGC 7822 is a young star forming complex in the constellation of Cepheus.The complex encompasses the emission region designated Sharpless 171, and the young cluster of stars named Berkeley 59.
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Sofia Cederblad, 43 år i Degeberga på Tingsvägen 54 - Mrkoll

749. 5565. 251 800. 2 199 785. 22 198. 2011. 12 123.

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What's going on here? Cederblad 214 is a bright nebula and star-forming region in the wider SH2-171 area in Cepheus. It contains the star cluster Berkeley 59 (bottom-left of centre in this image). The complex is believed to be some 800–1000 parsecs distant, with the younger components aged no more than a few million years. Cederblad 214 - posted in Experienced Deep Sky Imaging: Here is Cederblad 214. Some images of this region are a wider view with the full NGC 7822 and Cederblad complex.

About this Object: The young stellar association Cepheus OB4 lies in a region of bright nebulosity known as NGC 7822 and S 171. The fainter northern arch of nebulosity is designated NGC 7822(North up East left) and the brighter southern cloud is designated S 171 (Sharpless, 1959) or alternatively Cederblad 214. Cederblad 214.