Observed dynamical parameters of the disk clusters of the LMC. I

Details Observed dynamical parameters of the disk clusters of the LMC. I Observed dynamical parameters of the disk clusters of the LMC. I

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...68..147k&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 68, no. 1, Feb. 1987, p. 147-169.

Astronomy and Astrophysics

Astrophysics

24

Disk Galaxies, Globular Clusters, Magellanic Clouds, Star Distribution, Stellar Mass, Tables (Data)

Scientific paper

A study of the observed dynamical parameters of 32 globular clusters of the LMC disk has been carried out by means of star counts. The clusters were measured on a set of three plates (J, V, I) taken with the 1.2 m U.K. Schmidt Telescope. The derived tidal radii were all found to be large within a very narrow range. As a consequence the range of the total masses was found to be very narrow as well. These two parameters are large in comparison to those of the disk young clusters of our galaxy but they are similar to the dimensions of the halo galactic globulars.

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