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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
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) 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, 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
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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