Globular clusters, old and young
Creators
Description
The problem of similarity of and difference in the globular and scattered star clusters is considered. Star clusters in astronomy are related either to globular or to scattered ones according to the structure of Hertzsprung-Russell diagram constructed for star clusters, but not according to the appearance. The qlobular clusters in the Galaxy are composed of giants and subgiants, which testifies to the old age of the globular clusters. The Globular clusters in the Magellanic clouds are classified into ''red'' ones - similar to the globular clusters of the Galaxy, and ''blue'' ones - similar to them in appearance but differing extremely by the star composition and so by the age. The old star clusters are suggested to be called globular ones, while another name (''populous'', for example) is suggested to be used for other clusters similar to globular ones only in appearance
Additional details
Additional titles
- Original title (Russian)
- Шаровые скопления, старые и молодые
Publishing Information
- Journal Title
- Zemlya Vselennaya
- Journal Issue
- no.6
- Series
- Zemlya Vselennaya.
- ISSN
- 0044-3948
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 16048129
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- HERTZSPRUNG-RUSSELL DIAGRAM; STAR CLUSTERS
- Descriptors DEC
- DIAGRAMS; INFORMATION