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Ciencias Astronómicas
6
Galaxies: star clusters
3
Globular clusters: general
3
Galaxies: haloes
2
Galaxies: individual: NGC 4649
2
Galaxies: star clusters: general
2
Física
1
Galaxies: Star clusters
1
Galaxies: clusters: general
1
Galaxies: elliptical and lenticular
1
Galaxies: elliptical and lenticular, cD
1
Galaxies: formation
1
Galaxies: general
1
Galaxies: halos
1
Galaxies: individual
1
Galaxies: kinematics and dynamics
1
Galaxies: photometry
1
Globular clusters: individual: NGC 1399
1
Globular clusters: individual: NGC 4486
1
NGC 1399
1
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1“... of the diffuse stellar populations in early-type galaxies if the number of clusters per unit stellar mass depends...”
Aportado por: SEDICI (UNLP)Articulo -
2“... by assuming that the number of globular clusters per associated diffuse stellar mass t is a function of total...”
Aportado por: SEDICI (UNLP)Articulo -
3por Bassino, Lilia Patricia, Faifer, Favio Raúl, Forte, Juan Carlos, Dirsch, B., Richtler, T., Geisler, D., Schuberth, Y.“... and up to a limiting radius where the areal density of blue globular clusters falls to 30 per cent...”
Publicado 2006
Aportado por: SEDICI (UNLP)Articulo -
4por Bridges, Terry, Gebhardt, Karl, Sharples, Ray, Faifer, Favio Raúl, Forte, Juan Carlos, Beasley, Michael A., Zepf, Stephen E., Forbes, Duncan A., Hanes, David A., Pierce, Michael“... find no rotation of the GC system, with an upper limit of ν/σ < 0.6 at a confidence level of 95 per...”
Publicado 2006
Aportado por: SEDICI (UNLP)Articulo -
5por Forbes, Duncan A., Faifer, Favio Raúl, Forte, Juan Carlos, Bridges, Terry, Beasley, Michael A., Gebhardt, Karl, Hanes, David A., Sharples, Ray, Zepf, Stephen E.“... candidate GCs. Our source list is greater than 90 per cent complete to a magnitude of i = 23.6, and has...”
Publicado 2004
Aportado por: SEDICI (UNLP)Articulo -
6por Faifer, Favio Raúl, Forte, Juan Carlos, Norris, Mark A., Bridges, Terry, Forbes, Duncan A., Zepf, Stephen E., Beasley, Mike, Gebhardt, Karl, Hanes, David A., Sharples, Ray M.“... contamination level of only ~10 per cent in our sample of GC candidates. Bimodal GC colour distributions...”
Publicado 2011
Aportado por: SEDICI (UNLP)Articulo