The core of the Canis Major galaxy as traced by red clump stars

The core of the Canis Major galaxy as traced by red clump stars

Source :

• Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2006-03.

Descripteurs français

• Pascal (Inist)
  • Amas ouvert, Asymétrie, Brillance surface, Combustion stellaire, Disque galactique, Déformation, Etoile rouge, Etoile séquence principale, Galaxies naines, Magnitude absolue, Modèle, Orbite, Plan galactique, Population stellaire, Simulation numérique, Structure galaxies, Système n corps, Système stellaire, Traceur.
• Wicri :
  • geographic : Monaco.

English descriptors

• KwdEn :
  • 2mass, 2mass point source catalogue, Absolute magnitude, Argo, Argo structure, Asymmetry, Bellazzini, Black line, Canis, Central surface brightness, Centre, Chemical composition, Clump stars, Cmds, Colour, Colour range, Colour window, Compact structure, Contamination, Continuous line, Continuous lines, Cored structure, Current models, Deformation, Densest part, Density difference, Density distributions, Density maps, Density scale, Different directions, Different distances, Different nature, Different tracers, Digital simulation, Direct comparison, Disc, Distance distribution, Distance estimates, Distance indicators, Distance scale, Djorgovski sosin, Dominant contributors, Dsph, Dwarf, Dwarf contamination, Dwarf galaxies, Dwarf galaxy, Dwarf galaxy remnant, Dwarf spheroidal galaxies, Dwarf stars, Elliptical shape, Evolutionary phase, Excellent agreement, Extinction, Extinction laws, Fractional density, Fundamental parameters, Fusi pecci, Galactic, Galactic centre, Galactic disc, Galactic disks, Galactic hemisphere, Galactic latitudes, Galactic longitude, Galactic model, Galactic origin, Galactic plane, Galactic planes, Galactic warp, Galactocentric, Galactocentric distance, Galactocentric distances, Galaxy, Galaxy structure, Gaussian distribution, Giant branch, Good agreement, Heliocentric, Heliocentric distance, Heliocentric distances, Ibata, Inner circle, Interesting point, Interstellar extinction, Irwin, Journal compilation, Large dwarf galaxy, Large range, Little effect, Longitude, Lower panel, Luminosity, Magnitude range, Main body, Main sequence stars, Main structures, Majewski, Major axis, Maps show, Maximum density, Metallicity, Middle panel, Milky, Mnras, Models, Monaco, Monoceros ring, Monte carlo realization, N body system, Negative residuals, Negligible effect, Northern hemisphere, Northern hemisphere density, Northern lobe, Number density, Number surface density, Observational evidence, Open clusters, Optical cmds, Orbits, Other hand, Other words, Outer disc, Overdensities, Overdensity, Penarrubia, Pezo corredoira, Photometric, Photometric errors, Photometric parallax, Photometry, Planar orbit, Present analysis, Present case, Present context, Present contribution, Present paper, Present study, Previous analyses, Previous papers, Quadrant, Real stars, Red stars, Renzini, Rescaled, Rescaled version, Residual, Roundish core, Same distance scale, Same longitude scale, Same range, Same selections, Same technique, Sinusoidal variation, Southern hemisphere, Southern hemisphere density, Southern overdensities, Southern overdensity, Southern warp, Spatial orientation, Standard deviation, Star, Star burning, Star counts, Stellar, Stellar component, Stellar population, Stellar populations, Stellar system, Stellar systems, Stellar warp, Strong overdensity, Surface brightness, Surface density, Synthetic cmds, Synthetic samples, Synthetic stars, Systemic velocity, Tidal disruption, Total luminosity, Total number, Tracer, Tracers, Upper panel, Usual spiral arms, Various analyses, Various distances, Velocity dispersion, Warp, Warp asymmetry, Warp model, Whole structure, Young stars, galaxies: dwarf, galaxy: structure, open clusters and associations: general, open clusters and associations: individual: Tombaugh 2, AM-2, Heffner 11.
• Teeft :
  • 2mass, 2mass point source catalogue, Absolute magnitude, Argo, Argo structure, Asymmetry, Bellazzini, Black line, Canis, Central surface brightness, Centre, Chemical composition, Clump stars, Cmds, Colour, Colour range, Colour window, Compact structure, Contamination, Continuous line, Continuous lines, Cored structure, Current models, Densest part, Density difference, Density distributions, Density maps, Density scale, Different directions, Different distances, Different nature, Different tracers, Direct comparison, Disc, Distance distribution, Distance estimates, Distance indicators, Distance scale, Djorgovski sosin, Dominant contributors, Dsph, Dwarf, Dwarf contamination, Dwarf galaxy, Dwarf galaxy remnant, Dwarf spheroidal galaxies, Dwarf stars, Elliptical shape, Evolutionary phase, Excellent agreement, Extinction, Extinction laws, Fractional density, Fundamental parameters, Fusi pecci, Galactic, Galactic centre, Galactic disc, Galactic hemisphere, Galactic latitudes, Galactic longitude, Galactic model, Galactic origin, Galactic plane, Galactic warp, Galactocentric, Galactocentric distance, Galactocentric distances, Galaxy, Gaussian distribution, Giant branch, Good agreement, Heliocentric, Heliocentric distance, Heliocentric distances, Ibata, Inner circle, Interesting point, Interstellar extinction, Irwin, Journal compilation, Large dwarf galaxy, Large range, Little effect, Longitude, Lower panel, Luminosity, Magnitude range, Main body, Main structures, Majewski, Major axis, Maps show, Maximum density, Metallicity, Middle panel, Milky, Mnras, Monaco, Monoceros ring, Monte carlo realization, Negative residuals, Negligible effect, Northern hemisphere, Northern hemisphere density, Northern lobe, Number density, Number surface density, Observational evidence, Open clusters, Optical cmds, Other hand, Other words, Outer disc, Overdensities, Overdensity, Penarrubia, Pezo corredoira, Photometric, Photometric errors, Photometric parallax, Photometry, Planar orbit, Present analysis, Present case, Present context, Present contribution, Present paper, Present study, Previous analyses, Previous papers, Quadrant, Real stars, Renzini, Rescaled, Rescaled version, Residual, Roundish core, Same distance scale, Same longitude scale, Same range, Same selections, Same technique, Sinusoidal variation, Southern hemisphere, Southern hemisphere density, Southern overdensities, Southern overdensity, Southern warp, Spatial orientation, Standard deviation, Star, Star counts, Stellar, Stellar component, Stellar populations, Stellar system, Stellar systems, Stellar warp, Strong overdensity, Surface brightness, Surface density, Synthetic cmds, Synthetic samples, Synthetic stars, Systemic velocity, Tidal disruption, Total luminosity, Total number, Tracer, Upper panel, Usual spiral arms, Various analyses, Various distances, Velocity dispersion, Warp, Warp asymmetry, Warp model, Whole structure, Young stars.

Abstract

• https://api.istex.fr/document/E87CC603800CDF9845D1D97A78DB0A10983D4482/fulltext/pdf
• https://api.istex.fr/document/53090C446B65FE4F67428E2969243FA31F062870/fulltext/pdf

Affiliations:

• Australie, France, Italie
• Alsace (région administrative), Grand Est, Nouvelle-Galles du Sud
• Strasbourg, Sydney
• Université de Sydney

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