Published November 1984 | Version v1
Journal article

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