J/A+A/545/A54       Danks 1, Danks 2, and RCW 79 variables        (Chene+, 2012)

Massive open star clusters using the VVV survey. I. Presentation of the data and description of the approach. Chene A.-N., Borissova J., Clarke J.R.A., Bonatto C., Majaess D.J., Moni Bidin C., Sale S.E., Mauro F., Kurtev R., Baume G., Feinstein C., Ivanov V.D., Geisler D., Catelan M., Minniti D., Lucas P., De Grijs R., Kumar M.S.N. <Astron. Astrophys., 545, A54-54 (2012)> =2012A&A...545A..54C 2012A&A...545A..54C
ADC_Keywords: Surveys ; Clusters, open ; Photometry, infrared Keywords: open clusters and associations: general - infrared: stars - surveys Abstract: The ESO Public Survey "VISTA Variables in the Via Lactea"' (VVV) provides deep multi-epoch infrared observations for unprecedented 562 sq. degrees of the Galactic bulge, and adjacent regions of the disk. The VVV observations will foster the construction of a sample of Galactic star clusters with reliable and homogeneously derived physical parameters (e.g., age, distance, and mass, etc.). In this first paper in a series, the methodology employed to establish cluster parameters for the envisioned database are elaborated upon by analysing four known young open clusters: Danks1, Danks2, RCW79, and DBS132. The analysis offers a first glimpse of the information that can be gleaned from the VVV observations for clusters in the final database. Wide-field, deep JHKs VVV observations, combined with new infrared spectroscopy, are employed to constrain fundamental parameters for a subset of clusters. Results are inferred from VVV near-infrared photometry and numerous low resolution spectra (typically more than 10 per cluster). The high quality of the spectra and the deep wide-field VVV photometry enables us to precisely and independently determine the characteristics of the clusters studied, which we compare to previous determinations. An anomalous reddening law in the direction of the Danks clusters is found, specifically E(J-H)/E(H-Ks)=2.20±0.06, which exceeds published values for the inner Galaxy. The G305 star forming complex, which includes the Danks clusters, lies beyond the Sagittarius-Carina spiral arm and occupies the Centaurus arm. Finally, the first deep infrared colour-magnitude diagram of RCW79 is presented, which reveals a sizeable pre-main sequence population. A list of candidate variable stars in G305 region is reported. This study demonstrates the strength of the dataset and methodology employed, and constitutes the first step of a broader study which shall include reliable parameters for a sizeable number of poorly characterised and/or newly discovered clusters. Description: We downloaded, from the VISTA Science Archive (VSA) website (http://horus.roe.ac.uk/vsa/), the stacked images of the individual 2048x2048 pixel exposures containing the three clusters presented in this paper. Danks 1 and Danks 2 both appear in VVV field d084, whilst RCW 79 falls in VVV field d086. These fields were observed twice in the ZYJHKs bands on 7 to 29 March 2010 (d084), and 18 March to 4 April 2010 (d086), with the VIRCAM camera mounted on the VISTA 4m telescope at Paranal Observatory . Objects: ---------------------------------------------------------- RA (ICRS) DE Designation(s) ---------------------------------------------------------- 13 12 27 -62 42.1 Danks 1 = Cl Danks 1 13 12 55 -62 40.9 Danks 2 = Cl Danks 2 13 39.9 -61 45 RCW 79 = RCW 79 13 12 18 -62 42.3 [DBS2003] 132 = [DBS2003] 132 ---------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 107 53 Position, photometry and spectral parameters table5.dat 43 89 List of variable candidates in Danks 1 and Danks 2 table6.dat 43 36 List of variable candidates in RCW 79 -------------------------------------------------------------------------------- See also: J/MNRAS/398/221 : UBVIJHK photometry towards (l=305,b=0) (Baume+, 2009) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 A11 --- Field [D1 D2 DBS2003 132] Field designation (1) 13- 14 A2 --- St [FS m] Status: field star (FS) or member (m) 16- 18 A3 --- --- [Obj ] 19- 20 I2 --- Obj ? Object ID number within the field (2) 22- 26 A5 --- D12 Davies et al. (2012MNRAS.419.1871D 2012MNRAS.419.1871D) designation of the star (3) 28- 29 I2 h RAh Right ascension (J2000) 31- 32 I2 min RAm Right ascension (J2000) 34- 39 F6.3 s RAs Right ascension (J2000) 41 A1 --- DE- Declination sign (J2000) 42- 43 I2 deg DEd Declination (J2000) 45- 46 I2 arcmin DEm Declination (J2000) 48- 52 F5.2 arcsec DEs Declination (J2000) 54- 58 F5.2 mag Vmag ? Johnson V magnitude (from Baume et al., 2009MNRAS.398..221B 2009MNRAS.398..221B, Cat. J/MNRAS/398/221) 60- 65 F6.3 mag Jmag ? Vista J magnitude 66- 70 F5.2 mag Hmag ? Vista H magnitude 72- 76 F5.2 mag Ksmag ? Vista Ks magnitude 78- 81 I4 km/s RV ? Radial velocity 83- 84 I2 km/s e_RV ? rms uncertainty on RV 86- 92 A7 --- SpType Spectral type determined from comparison with template spectra and UBV photometry 94- 97 F4.2 mag AK ? Absorption in K band 99-102 F4.2 mag e_AK ? rms uncertainty on AK 104-107 F4.2 kpc Dist ? Distance -------------------------------------------------------------------------------- Note (1): Field designations are: D1 = Danks 1 D2 = Danks 2 DBS2003 132 = [DBS2003] 132 Note (2): Stars are ordered as a function of their (non-)membership. Note (3): D1-NN or D2-NN, will be [DCT2012] DN-NN in Simbad -------------------------------------------------------------------------------- Byte-by-byte Description of file: table5.dat table6.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name Star name (1) 12- 20 F9.5 deg RAdeg Right ascension (J2000) 22- 31 F10.6 deg DEdeg Declination (J2000) 33- 37 F5.2 mag <Ksmag> Mean Ks magnitude 39- 43 F5.2 [mag] log(e_<Ksmag>) Log of mean Ks magnitude error -------------------------------------------------------------------------------- Note (1): D1-NNNN for Danks 1, D2-NNNN for Danks 2, RCW79-NNNN for RCW 79. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 03-Dec-2014
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