Aims. We quantify the intrinsic width of the red giant branches of three massive globular clusters in M31 in a search for metallicity spreads within these objects
International audienceContext: .Metal-poor globular clusters in the bulge are important tracers of e...
We have collected spectra of about 2000 red giant branch (RGB) stars in 19 Galactic globular cluste...
We present spectrophotometric data for 7 globular clusters and 2 open clusters in M31. The wide wave...
International audienceAims: We quantify the intrinsic width of the red giant branches of three massi...
Aims. We quantify the intrinsic width of the red giant branches of three massive globular clusters ...
This paper presents 3600—5400 Å integrated spectra of 19 globular clusters (or candidates) projected...
To derive the metallicities of M3 and M5, we used the shape of red giant branch, horizontal branch m...
Abstract We present metal abundance properties of 144 globular clusters associated with M81. These g...
Globular clusters generally appear in two subpopulations: a blue, metal-poor and a red, metal-rich o...
While it has been known for a long time that the sizes of globular clusters within our galaxy correl...
We carry out a joint spatial–kinematical–metallicity analysis of globular clusters (GCs) around the ...
We have collected spectra of about 2000 red giant branch (RGB) stars in 19 Galactic globular cluster...
We have obtained VI CCD photometry of the very metal-rich inner bulge globular clusters NGC 6528, NG...
We report the discovery of significant stellar substructure in the halo and outer disk of our neares...
The spatial metallicity distribution in the Galaxy, as depicted by the globular cluster system, is a...
International audienceContext: .Metal-poor globular clusters in the bulge are important tracers of e...
We have collected spectra of about 2000 red giant branch (RGB) stars in 19 Galactic globular cluste...
We present spectrophotometric data for 7 globular clusters and 2 open clusters in M31. The wide wave...
International audienceAims: We quantify the intrinsic width of the red giant branches of three massi...
Aims. We quantify the intrinsic width of the red giant branches of three massive globular clusters ...
This paper presents 3600—5400 Å integrated spectra of 19 globular clusters (or candidates) projected...
To derive the metallicities of M3 and M5, we used the shape of red giant branch, horizontal branch m...
Abstract We present metal abundance properties of 144 globular clusters associated with M81. These g...
Globular clusters generally appear in two subpopulations: a blue, metal-poor and a red, metal-rich o...
While it has been known for a long time that the sizes of globular clusters within our galaxy correl...
We carry out a joint spatial–kinematical–metallicity analysis of globular clusters (GCs) around the ...
We have collected spectra of about 2000 red giant branch (RGB) stars in 19 Galactic globular cluster...
We have obtained VI CCD photometry of the very metal-rich inner bulge globular clusters NGC 6528, NG...
We report the discovery of significant stellar substructure in the halo and outer disk of our neares...
The spatial metallicity distribution in the Galaxy, as depicted by the globular cluster system, is a...
International audienceContext: .Metal-poor globular clusters in the bulge are important tracers of e...
We have collected spectra of about 2000 red giant branch (RGB) stars in 19 Galactic globular cluste...
We present spectrophotometric data for 7 globular clusters and 2 open clusters in M31. The wide wave...
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