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Globular Cluster
(redirected from Globular clusters)

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globular cluster: see star cluster star cluster, a group of stars near each other in space and resembling each other in certain characteristics that suggest a common origin for the group. Stars in the same cluster move at the same rate and in the same direction.
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globular cluster

Any large group of old, Population II (see Populations I and II) stars closely packed in a symmetrical, somewhat spherical form. About 150 have been identified in the Milky Way Galaxy. Most are distributed in a spherical volume above and below the Galaxy's disk (see galactic halo). Globular clusters contain many more stars (10,000–1,000,000) than open clusters do and can be several hundred light-years in diameter. Because they are so distant from the solar system, most are not visible to the unaided eye. Omega Centauri and a few others can be seen without a telescope as hazy patches of light.


Globular Cluster 

a tightly packed group of stars that can be seen in a small section of the sky, consisting of stars that are close to one another in space and characterized by the spherical shape of the distribution of the stars. Two of the globular clusters closest to us, with a myriad of stars, are located in the constellations Hercules and Centaurus. (SeeSTAR CLUSTER.)



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The two greatest globular clusters lie in the southern hemisphere, Omega Centauri and 47 Tucana.
They provide excellent opportunities for astronomers to study the elusive globular clusters lurking within.
Papers are in sections on hot subdwarfs in galaxies and globular clusters, atmospheres and evolution, binaries, and pulsating sdB/O stars.
 
 
 
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