Cl* NGC 5139 SAW V199 , the SIMBAD biblio

Cl* NGC 5139 SAW V199 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST04:30:48


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Title First 3 Authors
1996A&AS..120..139K viz 45 78 The optical gravitational lensing experiment. Variable stars in globular clusters. I. Fields 5139A-C in ω Centauri. KALUZNY J., KUBIAK M., SZYMANSKI M., et al.
1999A&A...346..487P 38 9 The light curves of the short-period variable stars in ω Centauri. PORETTI E.
2000A&A...359..597R viz 163 49 SX Phe stars in globular clusters. RODRIGUEZ E. and LOPEZ-GONZALEZ M.J.
2000PASP..112.1096M 57 25 The identification of pulsation modes of high-amplitude δ Scuti stars in ω Centauri and the Carina galaxy. McNAMARA D.H.
2001ApJ...554.1124S 170 33 Linear nonadiabatic properties of SX Phoenicis variables. SANTOLAMAZZA P., MARCONI M., BONO G., et al.
2003MNRAS.345...86O 121 13 Cluster AgeS Experiment (CASE): RR Lyrae stars from the globular cluster ω Centauri as standard candles. OLECH A., KALUZNY J., THOMPSON I.B., 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.
2008ApJ...685..947P viz 15       D               1 157 37 Variable stars in the Fornax dSph galaxy. II. Pulsating stars below the horizontal branch. PORETTI E., CLEMENTINI G., HELD E.V., 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.
2012MNRAS.419..342C viz 15       D               1 351 50 SX Phoenicis period–luminosity relations and the blue straggler connection. COHEN R.E. and SARAJEDINI A.
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.
2025MNRAS.539.3381D 112       D         F     3 66 ~ Asteroseismology of blue stragglers in ω Centauri: the case of five double-mode radial SX Phoenicis pulsators. DASZYNSKA-DASZKIEWICZ J., WALCZAK P., GORA P., et al.

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