2MASS J13262921-4731092 , the SIMBAD biblio

2MASS J13262921-4731092 , the SIMBAD biblio (25 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST13:59:15

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1977MNRAS.178..345L 19 35 Near infrared photometry of globular clusters. V. Structure on the giant branch of omega Centauri. LLOYD EVANS T.
1980ApJ...235..452P 72 103 The spread in CO absorption and effective temperature among the giants in omega Centauri. PERSSON S.E., FROGEL J.A., COHEN J.G., et al.
1983MNRAS.204..975L 28 ~ S stars in omega Centauri. LLOYD EVANS T.
1986ApJ...305..698C 70 34 The C, N, and O abundances of giant stars in omega Centauri. COHEN J.G. and BELL R.A.
1986SAAOC..10....1L 214 ~ Spectroscopic data for globular cluster giants. II. Giant stars in omega Centauri. LLOYD EVANS T.
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 3122 140 A proper motion study of the globular cluster ω Centauri. VAN LEEUWEN F., LE POOLE R.S., REIJNS R.A., et al.
2000ApJ...534L..83P 8 9 225 New evidence for the complex structure of the red giant branch in ω Centauri. PANCINO E., FERRARO F.R., BELLAZZINI M., et al.
2002A&A...383..491T 40 51 Accretion of gas by globular cluster stars. THOUL A., JORISSEN A., GORIELY S., et al.
2002ApJ...568L.101P 17       D               1 11 117 High-resolution spectroscopy of metal-rich giants in ω Centauri: first indication of type Ia supernova enrichment. PANCINO E., PASQUINI L., HILL V., et al.
2002ApJ...569..984V 15 26 Abundance patterns of the s stars in ω Centauri. VANTURE A.D., WALLERSTEIN G. and SUNTZEFF N.B.
2002ApJ...573L..95F 3 4 43 Discovery of an accreted stellar system within the globular cluster ω Centauri. FERRARO F.R., BELLAZZINI M. and PANCINO E.
2003ApJ...591..916O 3 7 67 A near-infrared spectroscopic screening of the red giant populations in ω Centauri. ORIGLIA L., FERRARO F.R., BELLAZZINI M., et al.
2004AJ....127..958R viz 41 58 CCD photometry of the globular cluster ω Centauri. II. Stellar populations and age-metallicity relation. REY S.-C., LEE Y.-W., REE C.H., et al.
1983SAAOC...7...96L 90 10 Spectroscopic data for globular cluster giants. 1. Stars of the red giant tip. LLOYD EVANS T.
2007ApJ...661L.155P viz 15       D               650 34 The rotation of subpopulations in ω Centauri. PANCINO E., GALFO A., FERRARO F.R., et al.
2008ApJ...681.1505J viz 15       D               1 183 43 Fe and Al abundances for 180 red giants in the globular cluster omega Centauri (NGC 5139). JOHNSON C.I., PILACHOWSKI C.A., SIMMERER J., et al.
2010ApJ...714.1001S 15       D               2 53 13 Abundances of C, N, sr, and ba on the red giant branch of ω Centauri. STANFORD L.M., DA COSTA G.S. and NORRIS J.E.
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.
2013ApJ...769...40C viz 15       D               1 113 21 Potassium in globular cluster stars: comparing normal clusters to the peculiar cluster NGC 2419. CARRETTA E., GRATTON R.G., BRAGAGLIA A., et al.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.

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