The structure of the system of long-period variable stars

Details The structure of the system of long-period variable stars The structure of the system of long-period variable stars

Publishing date

Oct 1979

URL

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979velen....q..95g&link_type=abstract

Journals

Leningradskii Universitet, Vestnik, Matematika, Mekhanika, Astronomiia, Oct. 1979, p. 95-99. In Russian.

Science

Astronomy and Astrophysics

Field

Astronomy

Additional info 3

Star Distribution, Stellar Structure, Variable Stars, Density Distribution, Milky Way Galaxy

Type

Scientific paper

Abstract

The data on long-period variables (P not less than 200d) given in the General Catalogue of Variable Stars are used to determine the structure of the LPV system. It is found that in the first approximation this system can be represented as a combination of objects belonging to a plane subsystem (beta of about 150 ps) and to an intermediate system (beta of about 500 ps). The two subsystems have about the same number of stars.

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