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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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