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NGC 1261

From Wikipedia, the free encyclopedia
Globular cluster in the constellation Horologium
NGC 1261
Observation data (J2000.0epoch)
ClassII[1]
ConstellationHorologium
Right ascension03h 12m 16.21s[2]
Declination–55° 12′ 58.4″[2]
Distance53.5 kly (16.4 kpc)[3]
Apparent magnitude (V)8.63[4]
Apparent dimensions (V)12.9
Physical characteristics
Absolute magnitude−7.81[5]
Mass3.41×105[6] M
Metallicity[Fe/H] = −1.38±0.14[5]dex
Estimated age10.24 Gyr[7]
Other designationsGCL 5,[4] ESO 155-SC11,Caldwell 87,Melotte 19
See also:Globular cluster,List of globular clusters

NGC 1261 (also known asCaldwell 87) is aglobular cluster of stars in the southernconstellation ofHorologium, first discovered by Scottish astronomerJames Dunlop in 1826. The cluster is located at a distance of 53kilolight-years from theSun, and 59 kilolight-years from theGalactic Center.[3] It is about 10.24[7] billion years old with 341,000[6] times themass of the Sun. The cluster does not display the normal indications ofcore collapse, but evidence suggests it may have instead passed through a post core-collapse bounce state within the past two billion years. The central luminosity density is 2.22 L·pc−3, which is low for a globular cluster.[8] Despite this, it has aShapley–Sawyer Concentration Class of II,[1] indicating a dense central concentration.

A total of 22RR Lyrae variables have been discovered in this cluster, along with twolong-period variables, threeSX Phoenicis variables, and aneclipsing binary.[9] It was determined to be anOosterhoff type I cluster, based on the periods of fourteen of the RR Lyrae variables.[10] 18 probableblue straggler candidates have been identified.[5]

References

[edit]
  1. ^abShapley, Harlow; Sawyer, Helen B. (August 1927), "A Classification of Globular Clusters",Harvard College Observatory Bulletin,849 (849):11–14,Bibcode:1927BHarO.849...11S.
  2. ^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.
  3. ^abPaust, Nathaniel E. Q.; et al. (February 2010), "The ACS Survey of Galactic Globular Clusters. VIII. Effects of Environment on Globular Cluster Global Mass Functions",The Astronomical Journal,139 (2):476–491,Bibcode:2010AJ....139..476P,doi:10.1088/0004-6256/139/2/476,hdl:2152/34371,S2CID 120965440.
  4. ^ab"NGC 1261".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2020-04-08.
  5. ^abcKravtsov, V.; et al. (June 2010), "Wide-field multi-color photometry of the Galactic globular cluster NGC 1261",Astronomy and Astrophysics,516: 8,arXiv:1005.0007,Bibcode:2010A&A...516A..23K,doi:10.1051/0004-6361/200913449,S2CID 55542820, A23.
  6. ^abBoyles, J.; et al. (November 2011), "Young Radio Pulsars in Galactic Globular Clusters",The Astrophysical Journal,742 (1): 51,arXiv:1108.4402,Bibcode:2011ApJ...742...51B,doi:10.1088/0004-637X/742/1/51,S2CID 118649860.
  7. ^abForbes, Duncan A.; Bridges, Terry (May 2010), "Accreted versus in situ Milky Way globular clusters",Monthly Notices of the Royal Astronomical Society,404 (3):1203–1214,arXiv:1001.4289,Bibcode:2010MNRAS.404.1203F,doi:10.1111/j.1365-2966.2010.16373.x,S2CID 51825384.
  8. ^Simunovic, Mirko; et al. (November 2014), "The Blue Straggler Star Population in NGC 1261: Evidence for a Post-core-collapse Bounce State",The Astrophysical Journal Letters,795 (1): 5,arXiv:1410.0693,Bibcode:2014ApJ...795L..10S,doi:10.1088/2041-8205/795/1/L10,S2CID 119294014, L10.
  9. ^Salinas, R.; et al. (September 2016), "An AO-assisted Variability Study of Four Globular Clusters",The Astronomical Journal,152 (3): 10,arXiv:1605.06517,Bibcode:2016AJ....152...55S,doi:10.3847/0004-6256/152/3/55,S2CID 119304354, 55.
  10. ^Wehlau, A.; Demers, S. (May 1977), "NGC 1261 and the Oosterhoff type I systems",Astronomy and Astrophysics,57:251–256,Bibcode:1977A&A....57..251W.

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