Detection of the Canis Major galaxy at (l;b) = (244°; −8°) and in the background of Galactic open clusters

Detection of the Canis Major galaxy at (l;b) = (244°; −8°) and in the background of Galactic open clusters

Source :

• Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2004-11.

Descripteurs français

• Pascal (Inist)
  • Age, Amas galactique, Amas ouvert, Catalogue astronomique, Diagramme magnitude couleur, Distance héliocentrique, Etoile séquence principale, Etude ciel, Galaxies naines, Isochrone, Module distance, Photométrie, Population stellaire, Position, Structure galaxies, Système stellaire.

English descriptors

• KwdEn :
  • 2mass, 2mass data, Age, Angular distance, Arcmin2, Astronomical catalogues, Asymmetry, Average reddening, Background population, Bellazzini, Blue plume, Canis, Carraro patat, Centre, Cluster, Cluster stars, Cmds, Color-magnitude diagrams, Colour, Colour range, Completeness factor, Completeness function, Data base, Deeper photometry, Different ranges, Different realizations, Distance estimates, Distance information, Distance moduli, Distance modulus, Distance scale, Dominant population, Dsph, Dwarf galaxies, Eld, Electronic form, Faint limit, Fainter magnitudes, Ferraro, Ferraro buonanno, Ferraro ibata, Field name, Full agreement, Future observations, Galactic, Galactic cluster, Galactic component, Galactic coordinates, Galactic disc, Galactic latitudes, Galactic model, Galactic plane, Galactic warp, Galaxy, Galaxy structure, Gilmore, Global model, Globular clusters, Good agreement, Guide star catalogue, Heavy dots, Heliocentric distance, High degree, Homogeneous data, Ibata, Inaf osservatorio astronomico, Incompleteness, Instrumental magnitudes, Interesting clues, Interstellar extinction, Irwin, Isochrone, Joint completeness factor, Kaluzny, Kassis, Large number, Latitude range, Local group, Lower panel, Magnitude axis, Main body, Main characteristics, Main population, Main sequence, Main sequence stars, Majewski, Maximum amplitude, Metallicity, Middle panel, Mnras, Modulus, Momany, Newberg, Open circles, Open cluster, Open clusters, Oschin schmidt telescope, Other hand, Overall appearance, Overall structure, Overdensity, Pezo corredoira, Photometric, Photometric parallax, Photometry, Positions, Possible effect, Present analysis, Present case, Present context, Previous section, Proper motions, Real warp, Reddening, Reddening differences, Reddening maps, Reddening values, Ring structure, Same area, Same assumptions, Same comparison, Same galactocentric distance, Same range, Same reddening, Schmidt telescope, Selection line, Sky surveys, Solid circles, Solid lines, Southern hemisphere, Star counts, Star experiments, Stars bluer, Stellar, Stellar content, Stellar population, Stellar populations, Stellar system, Stellar systems, Suitable control, Synthetic, Synthetic cmds, Synthetic sample, Synthetic star, Synthetic stars, Tangential velocity, Tentative detections, Theoretical isochrones, Thick disc, Tidal streams, Undesired contaminant, Unexpected population, Upper panel, Upper panels, Upper righthand panel, Various distances, Vertical lines enclose, Vertical plume, View arcmin2, Warp, Warp direction, Warp distribution, Warp model, Warp model encapsulated, Webda data base.
• Teeft :
  • 2mass, 2mass data, Angular distance, Arcmin2, Asymmetry, Average reddening, Background population, Bellazzini, Blue plume, Canis, Carraro patat, Centre, Cluster, Cluster stars, Cmds, Colour, Colour range, Completeness factor, Completeness function, Data base, Deeper photometry, Different ranges, Different realizations, Distance estimates, Distance information, Distance moduli, Distance modulus, Distance scale, Dominant population, Dsph, Eld, Electronic form, Faint limit, Fainter magnitudes, Ferraro, Ferraro buonanno, Ferraro ibata, Field name, Full agreement, Future observations, Galactic, Galactic component, Galactic coordinates, Galactic disc, Galactic latitudes, Galactic model, Galactic plane, Galactic warp, Galaxy, Gilmore, Global model, Globular clusters, Good agreement, Guide star catalogue, Heavy dots, Heliocentric distance, High degree, Homogeneous data, Ibata, Inaf osservatorio astronomico, Incompleteness, Instrumental magnitudes, Interesting clues, Interstellar extinction, Irwin, Isochrone, Joint completeness factor, Kaluzny, Kassis, Large number, Latitude range, Local group, Lower panel, Magnitude axis, Main body, Main characteristics, Main population, Main sequence, Majewski, Maximum amplitude, Metallicity, Middle panel, Mnras, Modulus, Momany, Newberg, Open circles, Open cluster, Open clusters, Oschin schmidt telescope, Other hand, Overall appearance, Overall structure, Overdensity, Pezo corredoira, Photometric, Photometric parallax, Photometry, Possible effect, Present analysis, Present case, Present context, Previous section, Proper motions, Real warp, Reddening, Reddening differences, Reddening maps, Reddening values, Ring structure, Same area, Same assumptions, Same comparison, Same galactocentric distance, Same range, Same reddening, Schmidt telescope, Selection line, Solid circles, Solid lines, Southern hemisphere, Star counts, Star experiments, Stars bluer, Stellar, Stellar content, Stellar population, Stellar populations, Stellar system, Suitable control, Synthetic, Synthetic cmds, Synthetic sample, Synthetic star, Synthetic stars, Tangential velocity, Tentative detections, Theoretical isochrones, Thick disc, Tidal streams, Undesired contaminant, Unexpected population, Upper panel, Upper panels, Upper righthand panel, Various distances, Vertical lines enclose, Vertical plume, View arcmin2, Warp, Warp direction, Warp distribution, Warp model, Warp model encapsulated, Webda data base.

Abstract

• https://api.istex.fr/document/AF21DADFDCB3D5BE23DFED751C6140C71FA8C767/fulltext/pdf

Affiliations:

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

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