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Clusters of Clusters: Globular Pairings
by Alan Whitman

Globular Groupings

Although we have reached the end of our tour, there are plenty of other pairs and chains of globulars in this region. In fact, M22 and NGC 6642 represent just one side of a compact trapezium of globulars that includes M28 and NGC 6638. If you find yourself under a moonless sky, perhaps at a star party, locate a spot with a good southern horizon and enjoy an evening with some of summer's clusters of globulars!

Globular Groupings
Name Const. R.A. (2000.0) Dec. (2000.0) Diam. Mag. Concen.
M4Sco16h 23.6m-26°32'35'5.4IX
NGC 6144Sco16h 27.3m-26° 02'17'9.0II
M9Oph17h 19.2m-18° 31'11'7.8VIII
NGC 6342Oph17h 21.2m-19° 35'  5'9.5IV
NGC 6356Oph17h 23.6m-17° 49'  8'8.2II
NGC 6522Sgr18h 03.6m-30° 02'  7'9.9VIII
NGC 6528Sgr18h 04.8m-30° 03'  5'9.6VIII
MGC 6642Sgr18h 31.9m-23° 29'  9'8.9V?
M22Sgr18h 36.4m-23° 54'33'5.2VIII

Note: the diameter (Diam.) and magnitude (Mag.) must be considered together when judging the difficulty of detecting any type of deep-sky object, but with globular clusters there is also a third important parameter — the Shapley-Sawyer concentration class (Concen.). Class I globulars are the most concentrated and have a high surface brightness, while Class XII are low-surface-brightness loose clusters.



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