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NGC 288 is a globular cluster in the constellation Sculptor. Its visual appearance was described by John Dreyer in 1888.[3] It is located about 1°.8 south-southest of the galaxy NGC 253, 15′ south of an 8th magnitude star, and encompassed by a half-circular chain of stars that opens on its southwest side.[1] It can be observed through binoculars.[1] It is not very concentrated and has a well resolved, large 3′ dense core that is surrounded by a much more diffuse and irregular 9′ diameter ring.[1] Peripheral members extend farther outward towards the south and especially southwest.[1]
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[edit] References
- ^ a b c d e f Kepple, George Robert; Glen W. Sanner (1998). The Night Sky Observer's Guide, Volume 2. Willmann-Bell, Inc., 365, 372. ISBN 0-943396-60-3.
- ^ a b c d SIMBAD Astronomical Database. Results for extended name search on NGC 288. Retrieved on 2007-02-10.
- ^ Dreyer, J. L. E. (1888). "A New General Catalogue of Nebulae and Clusters of Stars,being the Catalogue of the late Sir John F.W. Herschel, Bart., revised, corrected, and enlarged.". Memoirs of the Royal Astronomical Society 49: 1-237.
