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NGC 6584

From Wikipedia, the free encyclopedia
Globular cluster in the constellation Telescopium
NGC 6584
NGC 6584 as observed by the Hubble Space Telescope.
Observation data (J2000epoch)
ClassVIII
ConstellationTelescopium
Right ascension18h 18m 37.60s[1]
Declination–52° 12′ 56.8″[1]
Distance45000[2]
Apparent dimensions (V)7.9'
Physical characteristics
Metallicity[Fe/H] = −1.53±0.08[3]dex
Estimated age11.6±1.7 Gyr[3]
See also:Globular cluster,List of globular clusters

NGC 6584 is aglobular cluster in the constellationTelescopium that lies nearTheta Arae and is 45000 light-years distant.[2] It is anOosterhoff type I cluster, and contains at least 69 variable stars, most of which areRR Lyrae variables: 46 stars were identified as RRab variables; 15 as RRc variables, 1 RRe variable, 4 eclipsing binaries and 3 long period variables.[4] NGC 6584 is about 4 kpc from theGalactic Center and about 2.7 kpc from the Galactic plane.[5]

As is typical for metal-poor globular clusters, NGC 6584 has an enhanced concentration ofalpha elements relative to iron.[3]

References

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  1. ^abGoldsbury, Ryan; et al. (December 2010), "The ACS Survey of Galactic Globular Clusters. X. New Determinations of Centers for 65 Clusters",The Astronomical Journal,140 (6):1830–1837,arXiv:1008.2755,Bibcode:2010AJ....140.1830G,doi:10.1088/0004-6256/140/6/1830,S2CID 119183070.
  2. ^abStreicher, Magda (August 2009)."A Spyglass Telescope"(PDF).Deepsky Delights.68: 168.Bibcode:2009MNSSA..68..168S. Retrieved29 September 2012.[permanent dead link]
  3. ^abcHigh-resolution Spectroscopic Abundances of Red Giant Branch Stars in NGC 6584 and NGC 7099
  4. ^Toddy, Joseph M.; Johnson, Elliott W.; Darragh, Andrew N.; Murphy, Brian W. (2012). "New Variable Stars in the Globular Cluster NGC 6584".Journal of the Southeastern Association for Research in Astronomy.6:63–71.arXiv:1205.1034.Bibcode:2012JSARA...6...63T.
  5. ^"Physical Parameters of Galactic Globular Clusters" by S. Djorgovski

External links

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  • Media related toNGC 6584 at Wikimedia Commons
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