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physical object > natural object > celestial body > collection of stars > star cluster > globular cluster > Oosterhoff Group globular cluster |
Oosterhoff Group globular cluster | ||||
subject | fact |
Oosterhoff Group globular cluster | has definition Globular cluster which differs in the period of transition between Bailey type ab and type c variables, the ratio of type c to type ab stars, in the metallicity of RR Lyrae stars, and in the mean period of the ab variables. | |
is a kind of globular cluster | ||
globular cluster | has diameter about 100 light-years | |
has orbit elongated, around the galactic center | ||
is a part of halo | ||
has age oldest stellar formation in the Galaxy | ||
has number of stars 105 to 106 | ||
has catalog globular cluster catalog | ||
has spectra low abundances of heavy elements | ||
has velocity very high | ||
has mass 104 to 106 Msun | ||
has location most are in the halo some are members of the thick disk | ||
physical object | has angular momentum | |
has momentum | ||
has temperature | ||
has volume | ||
has extent | ||
has material |
Kinds of Oosterhoff Group globular cluster :
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