Studies of the open star cluster M 11. 3. Analysis of the two-point correlation function of member stars

Details Studies of the open star cluster M 11. 3. Analysis of the two-point correlation function of member stars Studies of the open star cluster M 11. 3. Analysis of the two-point correlation function of member stars

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cha%26a..20..508y&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 20, Issue 4, p. 508-508.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The correlation functions for all member stars and for members stars of
given magnitude ranges can all be represented by a power-law.
Calculation of the autocorrelations and cross correlations shows that M
11 has experienced a certain amount of dynamical relaxation which shows
up in mass segregation in space.

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