The application of a correlation analysis to the study of the cepheid distribution in the LMC

Details The application of a correlation analysis to the study of the cepheid distribution in the LMC The application of a correlation analysis to the study of the cepheid distribution in the LMC

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..777k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Sept. 1989, p. 777-784. In Russian. In Russian. In Russian.

Statistics

Computation

4

Astronomical Models, Cepheid Variables, Magellanic Clouds, Star Distribution, Computational Astrophysics, Correlation, Spatial Distribution

Scientific paper

The correlation function was used to study the cepheid distribution in
the LMC. This distribution is shown to be nonuniform. A method for
determining the characteristic size of groups of cepheids is proposed.
This size is 200 pk. The size of the region in the LMC characterized by
a nonuniform cepheid distribution is at least 2-3 kpk.

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