Evaporation of stars from isolated, truncated globular clusters

Details Evaporation of stars from isolated, truncated globular clusters Evaporation of stars from isolated, truncated globular clusters

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aj....105..155j&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 105, no. 1, p. 155-167.

Astronomy and Astrophysics

Astronomy

23

Evaporation Rate, Fokker-Planck Equation, Globular Clusters, Stellar Mass Ejection, Massive Stars, Milky Way Galaxy, Velocity Distribution

Scientific paper

An analysis is conducted of the escape rate of stars from model clusters vs concentration and global mass function, together with a detailed calculation of the number of escaping stars for the model cluster in a way that accumulates the escapes from progressively larger radii. The fractional escape rate from multimass clusters is a strong function of the lower mass cutoff. Attention is given to the escape rates for the Galactic globular clusters M4, M5, M68, NGC 6752, and 47 Tuc.

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