Cl* NGC 5139 BPB 168094 , the SIMBAD biblio

Cl* NGC 5139 BPB 168094 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST09:10:11

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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
1902AnHar..38....1B 132 147 A discussion of variable stars in the cluster omega Centauri. BAILEY S.I.
1986AJ.....92..358N 62 22 A search for double-mode RR Lyrae stars in omega Centauri. NEMEC J.M., NEMEC A.F.L. and NORRIS J.
1993A&A...276...87C 149 10 On the mass of type-c RR Lyrae variables in globular clusters. CACCIARI C. and BRUZZI A.
1996PAZh...22..597S 284 ~ Identification and coordinates of variable stars in the globular cluster omega Centauri = NGC 5139. SHOKIN Y.A. and SAMUS' N.N.
1997A&AS..122..471K viz 171 58 The optical gravitational lensing experiment. Variable stars in globular clusters. II. Fields 5139D-F in ω Centauri. KALUZNY J., KUBIAK M., SZYMANSKI M., et al.
1997A&AS..125..343K viz 144 42 The optical gravitational lensing experiment. Variable stars in globular clusters. III. RR Lyrae stars and Pop. II Cepheids in ω Centauri. KALUZNY J., KUBIAK M., SZYMANSKI M., 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.
2000AJ....119.1824R viz 144 63 CCD photometry of the globular cluster ω Centauri. I. Metallicity of RR Lyrae stars from Caby photometry. REY S.-C., LEE Y.-W., JOO J.-M., et al.
2000AJ....120.2579C 147 72 The globular cluster ω Centauri and the Oosterhoff dichotomy. CLEMENT C.M. and ROWE J.
2001AJ....121..951J 128 25 Period changes in ω Centauri RR Lyrae stars. JURCSIK J., CLEMENT C., GEYER E.H., et al.
2004A&A...424.1101K viz 407 48 Cluster AgeS Experiment. Catalog of variable stars in the globular cluster ω Centauri. KALUZNY J., OLECH A., THOMPSON I.B., et al.
2006A&A...445..901A viz 225 12 Variable stars in nearby galaxies. VII. P-L relation in the BVRI bands of Cepheids in IC 1613. ANTONELLO E., FOSSATI L., FUGAZZA D., et al.
2006ApJ...640L..43S viz 77 40 New metallicities of RR Lyrae stars in ω Centauri: evidence for a non-He-enhanced metal-intermediate population. SOLLIMA A., BORISSOVA J., CATELAN M., et al.
2007MNRAS.382.1353V viz 15       D               1531 37 A spectral atlas of post-main-sequence stars in ω Centauri: kinematics, evolution, enrichment and interstellar medium. VAN LOON J.T., VAN LEEUWEN F., SMALLEY B., et al.
2009A&A...493..959B viz 15       D               1 343 78 Ground-based CCD astrometry with wide field imagers. III. WFI.2m proper-motion catalog of the globular cluster ω C Centauri. BELLINI A., PIOTTO G., BEDIN L.R., et al.
2014MNRAS.439.3765D viz 16       D               1 377 16 Mid-infrared period-luminosity relations for globular cluster RR Lyrae. DAMBIS A.K., RASTORGUEV A.S. and ZABOLOTSKIKH M.V.
2016AJ....152..170B viz 136       D     X         4 244 27 On the RR Lyrae stars in globulars. IV. ω Centauri optical UBVRI photometry. BRAGA V.F., STETSON P.B., BONO G., et al.
2017A&A...604A.120N viz 16       D               2 198 7 Near-IR period-luminosity relations for pulsating stars in ω Centauri (NGC 5139). NAVARRETE C., CATELAN M., CONTRERAS RAMOS R., et al.
2018AJ....155..137B viz 16       D               2 213 17 On the RR Lyrae stars in globulars. V. The complete near-infrared (JHKs) census of ω Centauri RR Lyrae variables. BRAGA V.F., STETSON P.B., BONO G., et al.
2019ApJ...870..115B viz 17       D               1 174 6 On a new method to estimate the distance, reddening, and metallicity of RR Lyrae stars using optical/near-infrared (B, V, I, J, H, K) mean magnitudes: ω Centauri as a first test case. BONO G., IANNICOLA G., BRAGA V.F., et al.
2019A&A...625A...1B viz 59       D     X         2 283 2 New near-infrared JHKs light-curve templates for RR Lyrae variables. BRAGA V.F., STETSON P.B., BONO G., et al.
2019ApJ...881..104M viz 17       D               1 141 ~ Chemical compositions of field and globular cluster RR Lyrae stars. II. ω Centauri. MAGURNO D., SNEDEN C., BONO G., et al.

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