Globular cluster populations in four early type Poststarburst galaxies

Recent observations of the bulge display a gradient of the mean metallicity and of [Ƚ/Fe] with distance from galactic plane.. Bulge regions away from the plane are less

but no common halo able to reproduce simultaneously the properties of red and blue GCs velocities of some blue GCs require very large apogalactic distances – recent

We aim at identifying the least massive population of the solar metallicity, young (120 Myr), nearby (133.5 pc) Pleiades star cluster with the ultimate goal of understanding

Abstract: This paper introduces jNEP: a general, flexible, and rigorous implementation of NEPs (the basic model) and some interestenting variants; it is specifically designed to

Second, the sample of less massive (M  ≤ 1.5 M  ) giant stars with planets covers the same mass range as the MS pro- genitors and subgiant stars where the metal signature has

In Figure 18 we present the ratio of the dust luminosity (L dust ) derived from the UV/optical SED fitting to the observed IR luminosity against the current specific SFR.. Objects

of Hubble type, and galaxy stellar mass, M ?. The goals are: 1) to characterize in detail the radial structure of stellar population properties of galaxies in the local universe; 2)

In this article, we study the null controllability of a linear system coming from a population dynamics model with age structuring and spatial diffusion (of Lotka-McKendrick type)..