Jump to content

NGC 6834

From Wikipedia, the free encyclopedia
NGC 6834
Observation data (J2000.0epoch)
Right ascension19h52m12.5s[1]
Declination+29° 24′ 29″[1]
Distance10,850ly(3,326.7pc)[2]
Apparent magnitude(V)7.8[3]
Apparent dimensions (V)12[2]
Physical characteristics
Radius6.1 ly
Estimated age65±18Myr[4]
Other designationsNGC 6834, C 1950+292[5]
Associations
ConstellationCygnus
See also:Open cluster,List of open clusters

NGC 6834is a young[6]open clusterofstarslocated about 10,850[2]light yearsfrom theSunin theconstellationCygnus.It was discovered on July 17, 1784, by Anglo-German astronomerWilliam Herschel.[7]The cluster has avisual magnitudeof 7.8, which is dimmed by 2.1 magnitudes due tointerstellar dust.[3]Half the cluster members lie within anangular radiusof6′.[2]

TheTrumpler classof this cluster isII 2 m,indicating it is medium-rich in stars (m) with a moderate brightness range (2) and little central concentration of the stars (II).[6]It has about 260 members[2]and an age of approximately 65 million years,[4]although estimates range from 50 to 80 million.[6]A total of fifteenB-typevariable starshave been detected in the cluster with fourBe stars.Five of the cluster members showhydrogen alphaemission, including aγ Casand twoλ Erivariables.[6]

References

[edit]
  1. ^abKerber, F.; et al. (September 2003)."Galactic Planetary Nebulae and their central stars. I. An accurate and homogeneous set of coordinates".Astronomy and Astrophysics.408(3): 1029–1035.Bibcode:2003A&A...408.1029K.doi:10.1051/0004-6361:20031046.
  2. ^abcdeCantat-Gaudin, T.; Anders, F. (January 2020). "Clusters and mirages: cataloguing stellar aggregates in the Milky Way".Astronomy & Astrophysics.633:22.arXiv:1911.07075.Bibcode:2020A&A...633A..99C.doi:10.1051/0004-6361/201936691.S2CID208138247.A99.
  3. ^abCrossen, Craig; Rhemann, Gerald (2012).Sky Vistas: Astronomy for Binoculars and Richest-Field Telescopes.Springer Vienna. p. 68.ISBN9783709106266.
  4. ^abPaunzen, E.; Netopil, M. (October 2006). "On the current status of open-cluster parameters".Monthly Notices of the Royal Astronomical Society.371(4): 1641–1647.arXiv:astro-ph/0607421.Bibcode:2006MNRAS.371.1641P.doi:10.1111/j.1365-2966.2006.10783.x.S2CID15047964.
  5. ^"NGC 6834".SIMBAD.Centre de données astronomiques de Strasbourg.Retrieved2022-01-07.
  6. ^abcdMathew, Blesson; et al. (September 2014). "Optical/IR studies of Be stars in NGC 6834 with emphasis on two specific stars".Research in Astronomy and Astrophysics.14(9): 1173–1192.arXiv:1408.6658.Bibcode:2014RAA....14.1173M.doi:10.1088/1674-4527/14/9/008.S2CID118378570.1173-1192.
  7. ^Seligman, Courtney."NGC Objects: NGC 6800 - 6849".Celestial Atlas.Retrieved2022-01-08.
[edit]
  • Media related toNGC 6834at Wikimedia Commons