Browsing by Author "Correnti, M."
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- ItemA low surface brightness halo surrounding the globular cluster NGC 5694(2011) Correnti, M.; Catelan, Márcio
- ItemExtended Main Sequence Turnoffs in Intermediate-Age Star Clusters : A Correlation Between Turnoff Width and Early Escape Velocity(2014) Goudfrooij, P.; Girardi, L.; Kozhurina-Platais, V.; Kalirai, J.; Platais, I.; Puzia, Thomas H.; Correnti, M.; Bressan, A.; Chandar, R.
- ItemKinematics of a globular cluster with an extended profile: NGC 5694(2015) Bellazzini, M.; Mucciarelli, A.; Sollima, A.; Catelan, Márcio; Dalessandro, E.; Correnti, M.; D'Orazi, V.; Cortés, C .; Amigo, P.
- ItemNew constraints on the star formation history of the star cluster NGC 1856(2015) Correnti, M.; Goudfrooij, P.; Puzia, Thomas H.; De Mink, S.
- ItemNGC 5694: another extra-galactic globular cluster(2013) Mucciarelli, A.; Bellazzini, M.; Catelan, Márcio; Amigo, P.; Correnti, M.; Cortés, C.; Dalessandro, E.; D'Orazi, V.We discuss the chemical composition of six giant stars of the outer Halo globular cluster NGC 5694, through the analysis of UVES@FLAMES high-resolution spectra. The cluster has an average iron content [Fe/H]=-1.83±0.01, solar-scaled [alpha /Fe] ratios and a very low Ba abundance ([Ba/Fe]=-0.71±0.06). These anomalous abundance patterns are different from those observed in other Halo globular clusters but similar to those of the metal-poor stars in typical dwarf spheroidal galaxies. These findings suggest an extra-galactic origin for NGC 5694, likely from a dwarf spheroidal galaxy....
- ItemOn the interpretation of sub-giant branch morphologies of intermediate-age star clusters with extended main sequence turnoffs(2015) Goudfrooij, P.; Girardi, L.; Rosenfield, P.; Bressan, A.; Marigo, P.; Correnti, M.; Puzia, Thomas H.
- ItemThe Strikingly Metal-rich Halo of the Sombrero Galaxy(2020) Cohen, R. E.; Goudfrooij, P.; Correnti, M.; Gnedin, O. Y.; Harris, W. E.; Chandar, R.; Puzia, Thomas H.; Sánchez Janssen, R.