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It has been known since the 1950's that the observed gas content of Galactic globular clusters (GCs) is 2-3 orders of magnitude less than the mass lost by stars between Galactic disk crossings.
The combination of optical and near-infrared (NIR) colours has the potential to break the age/metallicity degeneracy and offers a better metallicity sensitivity than optical colours alone.
We use abundances of Ca, O, Na, Al from high resolution UVES spectra of 200 red giants in 17 globular clusters (GCs) to investigate the correlation found by Lee et al. (2009) between chemical enrichme...
Spectroscopic Study of the Globular Clusters in M31。
Galactic Orbits of Globular Clusters in a Barred Galaxy。
Core Radius-Mass Evolution of Globular Clusters
Far-ultraviolet surveys of globular clusterssearching For the products of stellar collisions and near misses
Using x-rays to probe the compact binary content of Globular clusters
Compact binaries in globular clusters
Modeling eclipsing binaries in globular clusters
Physical parameters of RR Lyraes in globular clusters from long term CCD photometry。
A particular case of mass distribution in stellar systems, already described in the literature, is compared to the King model of mass distribution. For the cases which would correspond to the descri...
The estimates of the mass of the galaxy NGC 5128 based on the di erent mass tracers, globular clusters (GCs) and planetary nebulae (PNe), are presented. These estimates are compared with the estimat...
Based on the relevant available data, the distributions of masses and apparent magnitudes of stars belonging to globular star clusters are simulated. The simulations are aimed at examining the in°ue...

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