We use new WFC3 observations of the nearby grand-design spiral galaxy M83 to develop two independent methods for estimating the ages of young star clusters. The first method uses the physical extent and morphology of Hα emission to estimate the ages of
The photometric characterization of M33 star clusters is far from complete. In this paper, we presen...
Aims. We present a new technique to estimate the relative ages of multiple stellar populations hoste...
We investigated the absolute age of the Galactic globular cluster M71 (NGC 6838) using optical groun...
The newly installed Wide Field Camera 3 (WFC3) on the Hubble Space Telescope has been used to obtain...
We present a multi-wavelength photometric study of ~15,000 resolved stars in the nearby spiral galax...
We present a multi-wavelength photometric study of 15,000 resolved stars in the nearby spiral galaxy...
We present observations obtained with the Advanced Camera for Surveys on board the Hubble Space Tele...
We investigated the Galactic globular cluster M71 (NGC6838, [Fe/H]=-0.78) by using optical (u', g', ...
5 pages, 5 figures.International audienceThe determination of age is a critical component in the stu...
We study the stellar cluster population in two adjacent fields in the nearby, face-on spiral galaxy,...
The newly installed Wide Field Camera 3 (WFC3) on the Hubble Space Telescope has been used to obtain...
A long-standing problem when deriving the physical properties of stellar populations is the degenera...
The study of young massive clusters can provide key information for the formation of globular cluste...
The morphology of H II regions around young star clusters providesThe morphology of H II regions aro...
We report on the properties of 89 low-mass star clusters located in the vicinity of luminous young c...
The photometric characterization of M33 star clusters is far from complete. In this paper, we presen...
Aims. We present a new technique to estimate the relative ages of multiple stellar populations hoste...
We investigated the absolute age of the Galactic globular cluster M71 (NGC 6838) using optical groun...
The newly installed Wide Field Camera 3 (WFC3) on the Hubble Space Telescope has been used to obtain...
We present a multi-wavelength photometric study of ~15,000 resolved stars in the nearby spiral galax...
We present a multi-wavelength photometric study of 15,000 resolved stars in the nearby spiral galaxy...
We present observations obtained with the Advanced Camera for Surveys on board the Hubble Space Tele...
We investigated the Galactic globular cluster M71 (NGC6838, [Fe/H]=-0.78) by using optical (u', g', ...
5 pages, 5 figures.International audienceThe determination of age is a critical component in the stu...
We study the stellar cluster population in two adjacent fields in the nearby, face-on spiral galaxy,...
The newly installed Wide Field Camera 3 (WFC3) on the Hubble Space Telescope has been used to obtain...
A long-standing problem when deriving the physical properties of stellar populations is the degenera...
The study of young massive clusters can provide key information for the formation of globular cluste...
The morphology of H II regions around young star clusters providesThe morphology of H II regions aro...
We report on the properties of 89 low-mass star clusters located in the vicinity of luminous young c...
The photometric characterization of M33 star clusters is far from complete. In this paper, we presen...
Aims. We present a new technique to estimate the relative ages of multiple stellar populations hoste...
We investigated the absolute age of the Galactic globular cluster M71 (NGC 6838) using optical groun...