2MASS J13271417-4730390 , the SIMBAD biblio

2MASS J13271417-4730390 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST22:49:35


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Title First 3 Authors
1996A&AS..115..297L viz 823 5 The central field of ω Centauri. LYNGA G.
1996AJ....111.1913S 514 166 The abundance spread among giants and subgiants in the globular cluster omega Centauri. SUNTZEFF N.B. and KRAFT R.P.
1996ApJ...462..241N viz 558 209 The giant branch of ω Centauri. V. The calcium abundance distribution. NORRIS J.E., FREEMAN K.C. and MIGHELL K.J.
1997AJ....114.1087M viz 449 37 Radial velocities of southern stars obtained with the photoelectric scanner CORAVEL. VIII. Observations of 471 giant stars in omega Centauri. MAYOR M., MEYLAN G., UDRY S., et al.
2000A&A...360..472V viz 14       D               3122 140 A proper motion study of the globular cluster ω Centauri. VAN LEEUWEN F., LE POOLE R.S., REIJNS R.A., et al.
2006A&A...445..503R viz 15       D               1971 33 Radial velocities in the globular cluster ω Centauri. REIJNS R.A., SEITZER P., ARNOLD R., et al.
2007ApJ...661L.155P viz 15       D               650 34 The rotation of subpopulations in ω Centauri. PANCINO E., GALFO A., FERRARO F.R., et al.
2010ApJ...722.1373J viz 15       D               1 882 284 Chemical abundances for 855 giants in the globular cluster omega Centauri (NGC 5139). JOHNSON C.I. and PILACHOWSKI C.A.
2011ApJ...731...64M viz 15       D               1 306 136 Sodium-oxygen anticorrelation and neutron-capture elements in Omega Centauri stellar populations. MARINO A.F., MILONE A.P., PIOTTO G., et al.
2012ApJ...746...14M 15       D               1 85 93 The C+N+O abundance of ω Centauri giant stars: implications for the chemical-enrichment scenario and the relative ages of different stellar populations. MARINO A.F., MILONE A.P., PIOTTO G., et al.
2018MNRAS.478.1520B viz 16       D               1 11619 300 A catalogue of masses, structural parameters, and velocity dispersion profiles of 112 Milky Way globular clusters. BAUMGARDT H. and HILKER M.

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