J/MNRAS/386/447     RV catalogue of O-type stars in NGC 6231       (Sana+, 2008)

The massive star binary fraction in young open clusters I. NGC 6231 revisited. Sana H., Gosset E., Naze Y., Rauw G., Linder N. <Mon. Not. R. Astron. Soc. 386, 447 (2008)> =2008MNRAS.386..447S 2008MNRAS.386..447S
ADC_Keywords: Binaries, spectroscopic ; Radial velocities ; Stars, O Keywords: binaries: close - binaries: spectroscopic - binaries: general - stars: early-type - open clusters and associations: individual: NGC 6231 - open clusters and associations: Sco OB1 Abstract: We present the results of a long-term high-resolution spectroscopy campaign on the O-type stars in NGC 6231. We revise the spectral classification and multiplicity of these objects and we constrain the fundamental properties of the O-star population. Almost three quarters of the O-type stars in the cluster are members of a binary system. The minimum binary fraction is 0.63, with half the O-type binaries having an orbital period of the order of a few days. The eccentricities of all the short-period binaries are revised downward, and henceforth match a normal period-eccentricity distribution. The mass-ratio distribution shows a large preference for O+OB binaries, ruling out the possibility that, in NGC 6231, the companion of an O-type star is randomly drawn from a standard IMF. Obtained from a complete and homogeneous population of O-type stars, our conclusions provide interesting observational constraints to be confronted with the formation and early-evolution theories of O stars. Description: Journal of the spectroscopic observations of the NGC6231 O-type stars studied in the present paper. The two header lines indicate the considered spectral lines and the adopted rest wavelength (in Angstroms). The first column indicates the object considered. The second and third ones gives the heliocentric Julian dates at mid-exposure and the code of the instrumental setup. The following columns provide the heliocentric RVs (expressed in km/s) using various spectral lines. The last two columns provide the mean and 1-sigma dispersion computed, for a given date, over the quoted lines. Whenever appropriate, the mean and 1-sigma dispersion for individual lines are also given at the bottom of each sub-table. WARNING: We stress out that the mean and sigma provided for information only, and might not have a direct physical meaning nor can they necessarily be directly compared to one another. Indeed, the mean and sigma have been computed by processing, for each object, the available measurements for a given line. No correction for e.g. different numbers of measurements from one line to another was included (consequently averaging over different phases in a binary system). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3m.dat 176 13 Mean radial velocities table3d.dat 104 227 Radial velocity data for O stars in NGC 6231 -------------------------------------------------------------------------------- See also: J/A+A/315/384 : Binarity among B-stars in NGC 6231 (Raboud, 1996) J/A+A/325/167 : Geneva photometry in NGC 6231 (Raboud+ 1997) J/AJ/115/734 : NGC 6231 UBVRI and Hα photometry (Sung+ 1998) J/A+AS/137/233 : UBVI imaging photometry of NGC 6231 (Baume+, 1999) J/A+A/454/1047 : XMM view of NGC 6231 open cluster (Sana+, 2006) J/MNRAS/372/661 : XMM view of NGC 6231: OB stars (Sana+, 2006) Byte-by-byte Description of file: table3m.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Name Object Identifier 12 A1 --- m_Name [ps] p for primary, s for secondary 14- 18 F5.1 km/s HeI4026 ? Mean radial velocity measured on HeI4026 (r.w. 4026.072) (G2) 20- 24 F5.1 km/s SiIV4089 ? Mean radial velocity measured on SiIV4089 (r.w. 4088.863) (G2) 26- 31 F6.1 km/s HeI4144 ? Mean radial velocity measured on HeI4144 (r.w. 4143.759) (G2) 33- 38 F6.1 km/s HeI4388 ? Mean radial velocity measured on HeI4388 (r.w. 4387.928) (G2) 40- 45 F6.1 km/s HeI4471 ? Mean radial velocity measured on HeI4471 (r.w. 4471.512) (G2) 47- 51 F5.1 km/s MgII4481 ? Mean radial velocity measured on MgII4481 (r.w. 4481.228) (G2) 53- 58 F6.1 km/s HeII4542 ? Mean radial velocity measured on HeII4542 (r.w. 4541.590) (G2) 60- 65 F6.1 km/s HeII4686 ? Mean radial velocity measured on HeII5686 (r.w. 4685.682) (G2) 67- 72 F6.1 km/s HeI4921 ? Mean radial velocity measured on HeI4921 (r.w. 4921.929) (G2) 74- 79 F6.1 km/s HeI5876 ? Mean radial velocity measured on HeI5876 (r.w. 5875.620) (G2) 81- 86 F6.1 km/s HeI7065 ? Mean radial velocity measured on HeI7065 (r.w. 7065.190) (G2) 88- 93 F6.1 km/s MeanRV ? Mean radial velocity computed of the measured lines (G3) 95- 99 F5.1 km/s SigmaRV ? 1 sigma dispersion of the measured RVs (G3) 101-105 F5.1 km/s e_HeI4026 ? 1 sigma dispersion of HeI4026 mean velocity 107-111 F5.1 km/s e_SiIV4089 ? 1 sigma dispersion of SiIV4089 mean velocity 113-117 F5.1 km/s e_HeI4144 ? 1 sigma dispersion of HeI4144 mean velocity 119-123 F5.1 km/s e_HeI4388 ? 1 sigma dispersion of HeI4388 mean velocity 125-129 F5.1 km/s e_HeI4471 ? 1 sigma dispersion of HeI4471 mean velocity 131-135 F5.1 km/s e_MgII4481 ? 1 sigma dispersion of MgII4481 mean velocity 137-141 F5.1 km/s e_HeII4542 ? 1 sigma dispersion of HeII4542 mean velocity 143-147 F5.1 km/s e_HeII4686 ? 1 sigma dispersion of HeII5686 mean velocity 149-153 F5.1 km/s e_HeI4921 ? 1 sigma dispersion of HeI4921 mean velocity 155-159 F5.1 km/s e_HeI5876 ? 1 sigma dispersion of HeI5876 mean velocity 161-165 F5.1 km/s e_HeI7065 ? 1 sigma dispersion of HeI7065 mean velocity 167-171 F5.1 km/s e_MeanRV ? rms uncertainty on Mean (G3) 173-176 F4.1 km/s e_SigmaRV ? rms uncertainty on Sigma (G3) -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3d.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Name Object Identifier 12 A1 --- n_Name [ps] p for primary, s for secondary 14- 24 F11.3 d HJD Heliocentric Julian Date 26 A1 --- Inst [abcd] Instrument Setup Code (1) 28- 32 F5.1 km/s HeI4026 ? Radial velocity measured on HeI4026 (r.w. 4026.072) (G2) 34- 38 F5.1 km/s SiIV4089 ? Radial velocity measured on SiIV4089 (r.w. 4088.863) (G2) 40- 44 F5.1 km/s HeI4144 ? Radial velocity measured on HeI4144 (r.w. 4143.759) (G2) 46- 50 F5.1 km/s HeI4388 ? Radial velocity measured on HeI4388 (r.w. 4387.928) (G2) 52- 56 F5.1 km/s HeI4471 ? Radial velocity measured on HeI4471 (r.w. 4471.512) (G2) 58- 62 F5.1 km/s MgII4481 ? Radial velocity measured on MgII4481 (r.w. 4481.228) (G2) 64- 68 F5.1 km/s HeII4542 ? Radial velocity measured on HeII4542 (r.w. 4541.590) (G2) 70- 74 F5.1 km/s HeII4686 ? Radial velocity measured on HeII5686 (r.w. 4685.682) (G2) 76- 80 F5.1 km/s HeI4921 ? Radial velocity measured on HeI4921 (r.w. 4921.929) (G2) 82- 86 F5.1 km/s HeI5876 ? Radial velocity measured on HeI5876 (r.w. 5875.620) (G2) 88- 92 F5.1 km/s HeI7065 ? Radial velocity measured on HeI7065 (r.w. 7065.190) (G2) 94- 98 F5.1 km/s MeanRV Mean RV computed of the measured lines for a given HJD (G3) 100-104 F5.1 km/s SigmaRV ? 1 sigma dispersion of the measured RVs on a given HJD (G3) -------------------------------------------------------------------------------- Note (1): Instrument Setup Code as follows: a = CAT+CES b = ESO1.5m + FEROS c = ESO/MPG2.2m + FEROS d = CTIO1.5m + BME -------------------------------------------------------------------------------- Global notes: Note (G2): r.w.: rest wavelength (in Angstroms) adopted to compute the RVs Note (G3): WARNING: the mean and sigma are provided for information only, and might not have a direct physical meaning nor can they necessarily be directly compared to one another. Indeed, the mean and sigma have been computed by processing the available measurements for a given date. No correction for e.g. different numbers of measurements from one date to another was included (consequently averaging over different lines, with possibly different systemic velocities). -------------------------------------------------------------------------------- Acknowledgements: Hugues Sana, hsana(at)eso.org References: Sana et al., 2001A&A...370..121S 2001A&A...370..121S (HD 152248) Sana et al., 2003A&A...405.1063S 2003A&A...405.1063S (CPD-41 7742) Sana et al., 2006MNRAS.371...67S 2006MNRAS.371...67S (HD152219) Sana et al., 2007ApJ...659.1582S 2007ApJ...659.1582S (CPD -41 7733) Sana et al., 2008NewA...13..202S 2008NewA...13..202S (HD 152218)
(End) Hugues Sana [ESO, Chile], Patricia Vannier [CDS] 16-Feb-2008
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