Search results for "Mass function"

showing 2 items of 22 documents

The Gaia-ESO Survey: The present-day radial metallicity distribution of the Galactic disc probed by pre-main-sequence clusters

2017

Full list of authors: Spina, L.; Randich, S.; Magrini, L.; Jeffries, R. D.; Friel, E. D.; Sacco, G. G.; Pancino, E.; Bonito, R.; Bravi, L.; Franciosini, E.; Klutsch, A.; Montes, D.; Gilmore, G.; Vallenari, A.; Bensby, T.; Bragaglia, A.; Flaccomio, E.; Koposov, S. E.; Korn, A. J.; Lanzafame, A. C. Smiljanic, R.; Bayo, A.; Carraro, G.; Casey, A. R.; Costado, M. T.; Damiani, F.; Donati, P.; Frasca, A.; Hourihane, A.; Jofré, P.; Lewis, J.; Lind, K.; Monaco, L.; Morbidelli, L.; Prisinzano, L.; Sousa, S. G.; Worley, C. C.; Zaggia, S.

Initial mass functionastro-ph.SRMetallicityMilky Wayastro-ph.GAFOS: Physical sciencesstars:abundancesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesevolution [Galaxy]Galaxy: diskpre-main sequence [Stars]0103 physical sciencesCluster (physics)Astrophysics::Solar and Stellar Astrophysicsgalaxy:disk010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBPhysicsGalaxy: evolutiongeneral [Open clusters and associations]010308 nuclear & particles physicsStar formationstars: abundances; stars: pre-main sequence; Galaxy: abundances; Galaxy:disk; Galaxy: evolution; open clusters and associations: generalStars: abundancesabundances [Galaxy]galaxy:evolutionAstronomy and AstrophysicsOpen clusters and associations: generalAstrophysics - Astrophysics of GalaxiesSupernovaAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)abundances [Stars]stars:pre-main sequenceChamaeleonStars: pre-main sequenceGalaxy: abundancesAstrophysics::Earth and Planetary Astrophysicsdisk [Galaxy]galaxy:abundancesopen clusters and associations:generalOpen cluster
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The Gaia-ESO Survey: membership and initial mass function of the. Velorum cluster

2016

Understanding the properties of young open clusters, such as the Initial Mass Function (IMF), star formation history and dynamic evolution, is crucial to obtain reliable theoretical predictions of the mechanisms involved in the star formation process. We want to obtain a list, as complete as possible, of confirmed members of the young open cluster Gamma Velorum, with the aim of deriving general cluster properties such as the IMF. We used all available spectroscopic membership indicators within the Gaia-ESO public archive together with literature photometry and X-ray data and, for each method, we derived the most complete list of candidate cluster members. Then, we considered photometry, gra…

Initial mass functionStars: luminosity function mass functionStars: formationFOS: Physical sciencesTechniques: spectroscopicOpen clusters and associations: individual: γVelorum; Stars: formation; Stars: luminosity function mass function; Stars: pre-main sequence; Techniques: radial velocities; Techniques: spectroscopic; Astronomy and Astrophysics; Space and Planetary ScienceAstrophysicsStars: luminosity function01 natural sciencesstars: pre-main sequence / open clusters and associations: individual: γVelorum / stars: formation / stars: luminosity functionPhotometry (optics)stars: pre-main sequence / open clusters and associations: individual: γVelorum / stars: formation / stars: luminosity function mass function / techniques: radial velocities / techniques: spectroscopic0103 physical sciences010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Open clusters and associations: individual: γVelorumQCQBPhysics010308 nuclear & particles physicsStar formationTechniques: radial velocitieAstronomy and Astrophysicsmass function / techniques: radial velocities / techniques: spectroscopicAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesAstrophysics - Solar and Stellar AstrophysicsYoung populationmass functionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Techniques: radial velocitiesopen clusters and associations: individual: gamma VelorumStars: pre-main sequenceOpen cluster
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