stjärnhop, både nebulosan och stjämhopen har fått namnet IC 5146 trots att originalbeskrivningen i J L E. Dreyers Index Catalogue endast nämner nebulosan.

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We provide a first look at the results of the Herschel Gould Belt survey toward the IC 5146 molecular cloud and present a preliminary analysis of the filamentary structure in this region. The column density map, derived from our 70-500 μm Herschel data, reveals a complex network of filaments and confirms that these filaments are the main birth sites of prestellar cores.

NGC 4567-68. NGC 4548 (M 91). M45 Pleiaderna. NGC 6888. En del av svansens spets. NGC 1952 (M 1) - Crab Nebula.

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Fotograf: Rolf Johansson Teleskop: TS Optics 107mm APO Cocoon Nebula, IC 5146, is a reflection/ emission nebula and Caldwell object in Cygnus. It is about 3300 ly distant. Hidden inside the Cocoon is a newly  ARP 188 - Tadpole Galaxy, IC 5146 - Cocoon nebula, M31 - Andromeda galaxen, NGC 7000, IC 5070 - Nordamerikanska nebulosan. NGC6960 -  IC 1396. IC 1396. M31 Andromeda Galaxy. M33 Triangulum Galaxy.

IC 5146 (tamén coñecida coma Caldwell 19, Sh 2-125, e a Nebulosa do Casulo) é unha nebulosa de reflexión [5] /emisión e tamén é un obxecto de Caldwell da constelación de Cygnus. IC 5146 fai referencia específica ó cúmulo estelar mentres que Sh2-125 fai referencia á nebulosa. [6]

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NOTES EMISSION-LINE STARS IN IC 5146* IC 5146 is the bright nebulosity surrounding the Bi V star BD+46°3474. Although emission-Ha. stars in IC 5146 

Although IC 5146’s fanciful name fits wonderfully with its visual appearance, what you may not know is the moniker is also very indicative of the star-birth process going on inside! When viewing IC 5146, dark nebula Barnard 168 (B168) is an inseparable part of the experience, forming a dark lane that surrounds the cluster and projects westward forming the appearance of a trail behind the Cocoon. Posted in Uncategorized Post navigation. IC 1396 – Elephant’s Head.

IC5146 also known as The Cocoon Nebula is a reflection/emission nebula in the constellation Cygnus. This an active star-forming region. There is also a dark nebula B168 that surrounds the cluster. IC 5070 . Introduction | Map | My Best Own Photos | My Own Observations | References || Appendix: My Own Photos. On this page I collect my observations of the galactic emission nebula IC 5146 (Cocoon Nebula) in the constellation Cepheus..
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The Cocoon nebula – IC 5146. OC. Amateur/Processed. 1 comment.
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Key words: astrochemistry – dust, extinction – infrared: ISM – ISM: individual objects (IC 5146) – ISM: molecules. Online-only material: color figures. 1.

IC 5148 - planetarisk nebula i stjärnbild Gruis Typ: PN - Närliggande objekt: IC 5146, IC 5147, IC 5149, IC 5150. 74HC4538AD, MOT. 20. 74HC4538AD MIN#1000 ICs 74HC4538MUTIVIBRTDUA, IC, 2660.

IC 5146 - Cocoon. Specialfält. Objekt: IC5146 Cocoon Datum: 2006-09-09. Teleskop/optik: TMB 100 f8. Filter: Astronomik H-alpha. Film/Kamera: SXV-H9

This wide field image (by Adam Block/NOAO/AURA/NSF) well shows its position in the Milky Way at the end of the dark lane B 168 . According to "Star Clusters", by Brent Archinal and Steven Hynes , the open cluster Collinder 470 is 'involved' with IC 5146, but is not equal to IC 5146, and is cataloged as a separate object. Three-color photoelectric and photographic observations of stars in IC 5146 have been obtained to about V = 17. The color-magnitude diagram, like those for NGC 2264, NGC 6530, and the Orion Nebula cluster, consists of a normal main sequence from B1 to about A0, beyond which the stars lie above the main sequence and are presumably still in the gravitational contraction stage. Query : IC 5146 C.D.S.

It is your springboard to informative daytime tours, nighttime stargazing programs, fascinating exhibits, a terrific gift shop, and beautiful panoramic mountaintop views! Query : IC 5146 35 : C.D.S. - SIMBAD4 rel 1.7 - 2021.03.28CEST11:29:57 Available data : Basic data • Identifiers • Plot & images • Bibliography • Measurements • External archives • Notes • Annotations . Basic data : IC 5146 35 We extend the well established classification method of the Spitzer Legacy teams to archived WISE observations. We have adopted 2MASS photometry as a “standard catalogue” for comparisons.