The spatial structure of the globular cluster M12

Details The spatial structure of the globular cluster M12 The spatial structure of the globular cluster M12

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65...41p&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Jan.-Feb. 1988, p. 41-57. In Russian.

Astronomy and Astrophysics

Astronomy

4

Globular Clusters, Stellar Magnitude, Stellar Structure, Astronomical Photometry, Least Squares Method, Space Density, Spatial Distribution

Scientific paper

The spatial structure of M12 is examined with respect to different star magnitude intervals and the limiting star magnitude B down to which the star counts are made. The study was performed on the basis of astrometric and photometic measurements of two plates obtained with the 2-m reflecting telescope at Rozhen observatory in Bulgaria. It is shown that the radii of the cluster zones described by Kholopov increase systematicaly with B, following the same law below the transition region between the subgiant branch and the main-sequence turnooff.

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