J/ApJ/661/L155      Radial velocities RGB stars in omega Cen   (Pancino+, 2007)

The rotation of subpopulations in ω Centauri. Pancino E., Galfo A., Ferraro F.R., Bellazzini M. <Astrophys. J., 661, L155-L158 (2007)> =2007ApJ...661L.155P 2007ApJ...661L.155P
ADC_Keywords: Clusters, globular ; Stars, giant ; Radial velocities Keywords: globular clusters: individual (NGC 5139) - techniques: radial velocities Abstract: We present the first result of the Ital-FLAMES survey of red giant branch (RGB) stars in omega Cen. Radial velocities with a precision of ∼0.5km/s are presented for 650 members of omega Cen observed with FLAMES-GIRAFFE at the Very Large Telescope. Description: Observations were done with FLAMES at the ESO VLT in Paranal, Chile, between 2003 May 22 and 28, within the Guaranteed Observing Time of the Ital-FLAMES Consortium. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 60 649 Radial Velocity Measurements -------------------------------------------------------------------------------- See also: J/A+A/360/472 : Proper motions in omega Centauri (van Leeuwen+, 2000) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 6 I6 --- WFI Star Name, Cl* NGC 5139 WFI NNNNNN in Simbad (1) 8- 18 F11.7 deg RAdeg Right Ascension in decimal degrees (J2000) (2) 20- 30 F11.7 deg DEdeg Declination in decimal degrees (J2000) (2) 32- 37 F6.3 mag Bmag Johnson B band magnitude (1) 39- 44 F6.3 mag Icmag Cousins I band magnitude (1) 46- 52 F7.3 km/s HRV Heliocentric Radial Velocity 54- 58 F5.3 km/s e_HRV Error on HRV 60 I1 --- Pop Population (3) -------------------------------------------------------------------------------- Note (1): From Pancino et al. (2000ApJ...534L..83P 2000ApJ...534L..83P) Note (2): Derived using van Leeuwen at al. (2000, Cat. J/A+A/360/472). Note (3): Population classification according to Pancino et al. (2000ApJ...534L..83P 2000ApJ...534L..83P, 2003MNRAS.345..683P 2003MNRAS.345..683P) as follows: 1 = RGB-MP, the most metal-poor component at [Ca/H]~-1.4. 2 = RGB-MInt, the metal intermediate component 3 = RGB-a, the extreme metal-rich component -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 15-Apr-2009
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