Proper motion L and T dwarf candidate members of the Pleiades

Proper motion L and T dwarf candidate members of the Pleiades

Source :

• Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2007-07-01.

Descripteurs français

• Pascal (Inist)
  • Amas ouvert, Amas stellaire, Couleur, Diagramme magnitude couleur, Etoile faible masse, Modèle théorique, Mouvement propre, Naine brune, Pléiades.

English descriptors

• KwdEn :
  • Annulus, Arcsec, Background stars, Baraffe, Bihain, Blueward transition sequence, Bouvier, Bright stars, Brown dwarf, Brown dwarf stars, Candidate cluster members, Candidate members, Centroiding uncertainty, Cfht, Cfht survey, Cluster mass function, Cluster members, Cluster sequence, Color, Color-magnitude diagrams, Colour, Cond models, Control areas, Control circle, Core radius, Deg2, Dither pattern, Dusty isochrone, Dusty model, Dusty models, Dwarf, Dwarf candidates, Dwarf members, Effective temperature regime, Eld, Epoch difference, Evolutionary models, Fake stars, Good choice, Initial mass function, Jameson, Journal compilation, Lled, Lled circles, Lled diamonds, Lled squares, Lled triangles, Low-mass stars, Lowest mass, Luminosity function, Magnitude range, Mass spectrum, Mnras, Model isochrones, Moraux, National research council, Nextgen, Nextgen model, Object detection, Open circle, Open circles, Open clusters, Optical data, Osorio, Photometric, Photometric band, Photometry, Planetary mass, Pleiades, Pliz, Plzj, Point sources, Previous surveys, Probability annulus probability, Proper motion, Proper motion analysis, Proper motion measurement, Proper motion measurements, Proper motion members, Proper motion vector diagram, Proper motions, Radial method, Reference stars, Same pipeline, Same time, Selection criteria, Separate control clusters, Small points, Solid line, Spectral type, Spectral types, Star clusters, Star formation, Star formation process, Stauffer, Theoretical model, Theoretical models, Theoretical predictions, Ukirt, Vector point diagram, Velocity dispersion, Wfcam, Wfcam data, Wfcam tiles, Young ages, Young clusters, Zapatero, Zapatero osorio.
• Teeft :
  • Annulus, Arcsec, Background stars, Baraffe, Bihain, Blueward transition sequence, Bouvier, Bright stars, Brown dwarf, Candidate cluster members, Candidate members, Centroiding uncertainty, Cfht, Cfht survey, Cluster mass function, Cluster members, Cluster sequence, Colour, Cond models, Control areas, Control circle, Core radius, Deg2, Dither pattern, Dusty isochrone, Dusty model, Dusty models, Dwarf, Dwarf candidates, Dwarf members, Effective temperature regime, Eld, Epoch difference, Evolutionary models, Fake stars, Good choice, Initial mass function, Jameson, Journal compilation, Lled, Lled circles, Lled diamonds, Lled squares, Lled triangles, Lowest mass, Luminosity function, Magnitude range, Mass spectrum, Mnras, Model isochrones, Moraux, National research council, Nextgen, Nextgen model, Object detection, Open circle, Open circles, Optical data, Osorio, Photometric, Photometric band, Photometry, Planetary mass, Pleiades, Pliz, Plzj, Point sources, Previous surveys, Probability annulus probability, Proper motion, Proper motion analysis, Proper motion measurement, Proper motion measurements, Proper motion members, Proper motion vector diagram, Proper motions, Radial method, Reference stars, Same pipeline, Same time, Selection criteria, Separate control clusters, Small points, Solid line, Spectral type, Spectral types, Star formation, Star formation process, Stauffer, Theoretical models, Theoretical predictions, Ukirt, Vector point diagram, Velocity dispersion, Wfcam, Wfcam data, Wfcam tiles, Young ages, Young clusters, Zapatero, Zapatero osorio.

Abstract

• https://api.istex.fr/document/66F26ECD32AE3C9BB11064DD16821BBC7A74B980/fulltext/pdf
• https://api.istex.fr/document/58336ED7BE6B9107F04F3D53D9BD7991D5BBD833/fulltext/pdf

Affiliations:

• Australie, Espagne, France, Royaume-Uni
• Auvergne-Rhône-Alpes, Rhône-Alpes
• Grenoble
• Université Joseph Fourier

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