Compressive Effects on Globular Clusters by Gravitational Disk-Shocking

Details Compressive Effects on Globular Clusters by Gravitational Disk-Shocking Compressive Effects on Globular Clusters by Gravitational Disk-Shocking

Sep 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996pthph..96..537s&link_type=abstract

Progress of Theoretical Physics, Vol. 96, No. 3, pp. 537-547.

Physics

2

Scientific paper

Projected images of the Galactic globular clusters are not necessarily circular but elliptical in many cases. To study the possibility that the gravitational disk-shocking is the principal cause of the observed figures, we carry out a series of numerical experiments of disk-shocking on model clusters. We measure the axial ratios of the projected density contours of the model clusters, and find that the disk-shocking does not produce the values of axial ratios obtained by observations in the literature.

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