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NGC 6820 and NGC 6823

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(Redirected fromSh 2-86)
Emission nebula and star cluster in the constellation Vulpecula
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You can helpexpand this article with text translated fromthe corresponding article in French.Click [show] for important translation instructions.
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Emission Nebula NGC6820 with Open Cluster NGC6823
Emission nebula
NGC 6820/NGC 6823
Observation data: J2000.0epoch
Right ascension19h 42m 27.92s[1]
Declination+23° 05′ 14.7″[1]
Distance6,000[2] ly
Apparent dimensions (V)40arcmins
ConstellationVulpecula
DesignationsNebula (NGC 6820, Sh2-86)
See also:Lists of nebulae

NGC 6820 is a smallemission nebula near theopen clusterNGC 6823 inVulpecula. The reflection nebula and cluster are embedded in a large faint emission nebula calledSh 2-86. The whole area of nebulosity is often referred to as NGC 6820.[3]

M27, theDumbbell Nebula, is found three degrees to the east, andα Vulpeculae three degrees to the west.

Open star cluster NGC 6823 is about 50light-years across and lies about 6,000 light-years away. The center of the cluster formed about two million years ago and is dominated in brightness by a host of bright young blue stars. Outer parts of the cluster contain even younger stars.[2] It forms the core of theVulpecula OB1stellar association.[4]

Image gallery

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References

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  1. ^ab"NGC 6820".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2008-07-03.
  2. ^abNemiroff, R.; Bonnell, J., eds. (4 October 2004)."NGC 6823: Cloud Sculpting Star Cluster".Astronomy Picture of the Day.NASA. Retrieved2008-07-03.
  3. ^"Sharpless 86". Retrieved2017-11-19.
  4. ^Billot, N.; Noriega-Crespo, A.; Carey, S.; Guieu, S.; Shenoy, S.; Paladini, R.; Latter, W. (2010). "Young Stellar Objects and Triggered Star Formation in the Vulpecula Ob Association".The Astrophysical Journal.712 (2): 797.arXiv:1003.0866.Bibcode:2010ApJ...712..797B.doi:10.1088/0004-637X/712/2/797.S2CID 28961682.

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