0000000000890487

AUTHOR

Bertrand Lemasle

showing 2 related works from this author

On the nature of a shell of young stars in the outskirts of the Small Magellanic Cloud

2019

Understanding the evolutionary history of the Magellanic Clouds requires an in-depth exploration and characterization of the stellar content in their outer regions, which ultimately are key to tracing the epochs and nature of past interactions. We present new deep images of a shell-like over-density of stars in the outskirts of the Small Magellanic Cloud (SMC). The shell, also detected in photographic plates dating back to the fifties, is located at ~1.9 degr from the center of the SMC in the north-east direction.The structure and stellar content of this feature were studied with multi-band, optical data from the Survey of the MAgellanic Stellar History (SMASH) carried out with the Dark Ene…

Milky WayPopulationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicseducationLarge Magellanic Cloud010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicseducation.field_of_study010308 nuclear & particles physicsStar formationLocal GroupAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesStars[SDU]Sciences of the Universe [physics]Space and Planetary ScienceGlobular clusterAstrophysics of Galaxies (astro-ph.GA)Small Magellanic CloudAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Constraining the thin disc initial mass function using Galactic classical Cepheids

2016

Context: The Initial Mass Function (IMF) plays a crucial role on galaxy evolution and its implications on star formation theory make it a milestone for the next decade. It is in the intermediate and high mass ranges where the uncertainties of the IMF are larger. This is a major subject of debate and analysis both for Galactic and extragalactic science. Aims: Our goal is to constrain the IMF of the Galactic thin disc population using both Galactic Classical Cepheids and Tycho-2 data. Methods: For the first time the Besan\c{c}on Galaxy Model (BGM) has been used to characterise the Galactic population of the Classical Cepheids. We have modified the age configuration in the youngest populations…

Initial mass functionStar ClassificationCepheid variableMilky WayFOS: Physical sciencesClassificació dels estelsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences0103 physical sciencesGalaxy formation and evolutionAstrophysics::Solar and Stellar AstrophysicsDisc010303 astronomy & astrophysicsStellar densityComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxyGalaxies evolutionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Evolució de les galàxiesAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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