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The Gaia ultracool dwarf sample – II. Structure at the end of the main sequence
(Oxford University Press, 2019)
The old metal-poor open cluster ESO 92-SC05: accreted from a dwarf galaxy ?
(WILEY-BLACKWELL, 2008)
The study of old open clusters outside the solar circle can bring constraints on formation scenarios of the outer disc. In particular, accretion of dwarf galaxies has been proposed as a likely mechanism in the area. We use ...
Discovery of two distinct red clumps in NGC 419: a rare snapshot of a cluster at the onset of degeneracy
(WILEY-BLACKWELL PUBLISHING, INC, 2009)
Colour-magnitude diagrams (CMDs) of the Small Magellanic Cloud (SMC) star cluster NGC 419, derived from Hubble Space Telescope (HST)/Advanced Camera for Surveys (ACS) data, reveal a well-delineated secondary clump located ...
Self-consistent physical parameters for five intermediate-age SMC stellar clusters from CMD modelling
(EDP SciencesLes Ulis, 2014)
Context. Stellar clusters in the Small Magellanic Cloud (SMC) are useful probes for studying the chemical and dynamical evolution
of this neighbouring dwarf galaxy, enabling inspection of a large period covering over 10 ...
SMASHing the low surface brightness SMC
(Oxford University Press, 2020)
The periphery of the Small Magellanic Cloud (SMC) can unlock important information regarding galaxy formation and evolution in interacting systems. Here, we present a detailed study of the extended stellar structure of the ...
Recovery of the star formation history of the LMC from the VISTA survey of the Magellanic system
(EDP SCIENCES S A, 2009)
The VISTA near infrared survey of the Magellanic System (VMC) will provide deep YJK(s) photometry reaching stars in the oldest turn-off point throughout the Magellanic Clouds (MCs). As part of the preparation for the survey, ...
Open clusters: II fundamental parameters of B stars in Collinder 223, Hogg 16, NGC2645, NGC3114, and NGC6025
(Edp Sciences, 2015-05)
Context. The knowledge of accurate values of effective temperature, surface gravity, and luminosity of stars in open clusters is very important not only to derive cluster distances and ages but also to discuss the stellar ...