The star formation history in the far outer disc of M33

The star formation history in the far outer disc of M33

Source :

• Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2011-01-01.

Descripteurs français

• Pascal (Inist)
  • Abondance, Age, Brillance surface, Contenu stellaire, Diagramme magnitude couleur, Evolution galaxies, Formation stellaire, Galaxies disques, Galaxies spirales, Gauchissement, Groupe local, Masse stellaire, Modèle, Mélangeage, Métallicité, Rapport signal bruit.
• Wicri :
  • topic : Simulation.

English descriptors

• KwdEn :
  • Abundance, Age, Aparicio, Basti, Besancon model, Black line, Blue envelope, Blue peak, Blue plume, Bolometric corrections, Cent completeness, Cmds, Color-magnitude diagrams, Colour, Compelling evidence, Constant metallicity, Corbelli schneider, Corrections, Correlated errors, Cosmic rays, Cosmological, Cosmological context, Cosmological simulation, Cosmological simulations, Disc, Disc edge, Disc formation, Disc galaxies, Disc galaxy, Disc scalelengths, Disk galaxies, Distance modulus, Dominant population, Eld, Elmegreen parravano, Equal logarithmic intervals, Error bars, Foreground stars, Further details, Galaxy, Galaxy evolution, Gallart, Good agreement, Governato, Halo, Harris zaritsky, Hubble space telescope, Hybrid approach, Inner disc, Intermediate ages, Journal compilation, Large radii, Light curves, Linear combination, Local group, Magenta line, Magnitude range, Metallicities, Metallicity, Metallicity gradient, Metallicity spread, Mixing, Mnras, Models, Morphology, Older population, Optical image, Outer disc, Outer disc star formation history, Panels show, Parameter space, Photometric, Photometric errors, Private communication, Radial migration, Random search, Sarajedini, Scalelengths, Sharp drop, Signal-to-noise ratio, Simulation, Small fraction, Solar oxygen abundance, Solid lines, Spiral galaxies, Star, Star formation, Star formation history, Star tests, Steinmetz navarro, Stellar, Stellar content, Stellar mass, Stellar mass density, Stellar mass surface density, Stellar populations, Stellar surface density, Stock implementation, Such stars, Surface brightness, Synthetic cmds, Systematic error, Thick disc, Thick discs, Thin disc, Thin discs, Total model, Tting, Tting analysis, Tting region, Upper limit, Upper limits, Variable stars, Vertical clump, Vertical clump morphology, Warping, Younger ages, Youngest stars.
• Teeft :
  • Aparicio, Basti, Besancon model, Black line, Blue envelope, Blue peak, Blue plume, Bolometric corrections, Cent completeness, Cmds, Colour, Compelling evidence, Constant metallicity, Corbelli schneider, Corrections, Correlated errors, Cosmic rays, Cosmological, Cosmological context, Cosmological simulation, Cosmological simulations, Disc, Disc edge, Disc formation, Disc galaxies, Disc galaxy, Disc scalelengths, Distance modulus, Dominant population, Eld, Elmegreen parravano, Equal logarithmic intervals, Error bars, Foreground stars, Further details, Galaxy, Gallart, Good agreement, Governato, Halo, Harris zaritsky, Hubble space telescope, Hybrid approach, Inner disc, Intermediate ages, Journal compilation, Large radii, Light curves, Linear combination, Magenta line, Magnitude range, Metallicities, Metallicity, Metallicity gradient, Metallicity spread, Mnras, Morphology, Older population, Optical image, Outer disc, Outer disc star formation history, Panels show, Parameter space, Photometric, Photometric errors, Private communication, Radial migration, Random search, Sarajedini, Scalelengths, Sharp drop, Simulation, Small fraction, Solar oxygen abundance, Solid lines, Spiral galaxies, Star, Star formation, Star formation history, Star tests, Steinmetz navarro, Stellar, Stellar mass, Stellar mass density, Stellar mass surface density, Stellar populations, Stellar surface density, Stock implementation, Such stars, Synthetic cmds, Systematic error, Thick disc, Thick discs, Thin disc, Thin discs, Total model, Tting, Tting analysis, Tting region, Upper limit, Upper limits, Variable stars, Vertical clump, Vertical clump morphology, Younger ages, Youngest stars.

Abstract

• https://api.istex.fr/document/5BD198157C610D67687BE97A8A4CA2EAC530C4AC/fulltext/pdf

Affiliations:

• Australie, France, Royaume-Uni, États-Unis
• Alsace (région administrative), Californie, Grand Est, Nouvelle-Galles du Sud, Écosse
• Strasbourg, Sydney, Édimbourg
• Université d'Édimbourg, Université de Sydney

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