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J/AJ/138/159   NGC 6819 stellar radial-velocity and photometry    (Hole+, 2009)

WIYN open cluster study. XXIV. Stellar radial-velocity measurements in NGC 6819. Hole K.T., Geller A.M., Mathieu R.D., Platais I., Meibom S., Latham D.W. <Astron. J., 138, 159-168 (2009)> =2009AJ....138..159H
ADC_Keywords: Clusters, open ; Radial velocities ; Photometry, CCD ; Photometry, UBVRI ; Photometry, infrared Keywords: open clusters and associations: individual (NGC 6819) - techniques: radial velocities Abstract: We present the current results from our ongoing radial-velocity (RV) survey of the intermediate-age (2.4Gyr) open cluster NGC 6819. Using both newly observed and other available photometry and astrometry, we define a primary target sample of 1454 stars that includes main-sequence, subgiant, giant, and blue straggler stars, spanning a magnitude range of 11≤V≤16.5 and an approximate mass range of 1.1-1.6M. Our sample covers a 23 arcminute (13pc) square field of view centered on the cluster. We have measured 6571 radial velocities for an unbiased sample of 1207 stars in the direction of the open cluster NGC 6819, with a single-measurement precision of 0.4km/s for most narrow-lined stars. We use our RV data to calculate membership probabilities for stars with ≥3 measurements, providing the first comprehensive membership study of the cluster core that includes stars from the giant branch through the upper main sequence. We identify 480 cluster members. Additionally, we identify velocity-variable systems, all of which are likely hard binaries that dynamically power the cluster. Description: There are four sources of CCD BV photometry available to us for the cluster: RV98, Kalirai et al. (2001AJ....122..266K, hereafter K01), and two unpublished sets taken by members of the WOCS (WIYN Open Cluster Study) collaboration. The two sets of WOCS photometry were obtained at what was the KPNO and is now the WIYN7 0.9m telescope. In 1998 March, C. Dolan & R. Mathieu took BV CCD images to begin this RV project, hereafter called Phot98. These observations used the Tektronics CCD (T2KA) at f/7.5. The WOCS UBVRI study (hereafter Phot03) is based on images obtained with the SITe S2KB CCD camera (pixel size 0.60"), yielding an FOV of 20'. In total, we have observed 90 pointings on NGC 6819 over 35 separate observing runs on the WIYN 3.5m. The CfA RV measurements were obtained with two nearly identical instruments on the Multiple Mirror Telescope and the 1.5m Tillinghast Reflector at the Whipple Observatory atop Mt. Hopkins, Arizona. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 108 1305 The NGC 6819 WOCS photometry database table2.dat 102 1207 The NGC 6819 WOCS radial-velocity database
See also: J/MNRAS/358/795 : Variable stars in NGC 6819 field (Street+, 2005) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 6 I06 --- WOCS [1001/115030] WIYN Open Cluster Study identification (G1) 9- 14 F6.3 mag Vmag ? Phot98 project V band magnitude 16- 21 F6.3 mag B-V ? Phot98 project (B-V) color index 23- 28 F6.3 mag V-R ? Phot98 project (V-R) color index 30- 35 F6.3 mag V-I ? Phot98 project (V-I) color index 38- 43 F6.3 mag Vmag1 ? Phot03 project V band magnitude 45- 50 F6.3 mag B-V1 ? Phot03 project (B-V) color index 53- 58 F6.3 mag Vmag2 ? Rosvick & Vandenberg (1998AJ....115.1516R) V band magnitude 60- 65 F6.3 mag B-V2 ? Rosvick & Vandenberg (1998AJ....115.1516R) (B-V) color index 68- 73 F6.3 mag Vmag3 ? Kalirai et al. (2001AJ....122..266K) V band magnitude 75- 80 F6.3 mag B-V3 ? Kalirai et al. (2001AJ....122..266K) (B-V) color index 83- 88 F6.3 mag Jmag ? 2MASS J band magnitude 90- 95 F6.3 mag J-Ks ? 2MASS (J-Ks) color index 99-102 I4 --- A74 ? Auner (1974A&AS...13..143A) identification, <NGC 6819 NNN> in Simbad 106-108 I3 --- S72 ? Sanders (1972A&A....19..155S) identification, <[S72b] NGC 6819 NNN> in Simbad
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 6 I06 --- WOCS WIYN Open Cluster Study identification (G1) 8- 9 I2 h RAh Hour of Right Ascension (J2000) 11- 12 I2 min RAm Minute of Right Ascension (J2000) 14- 18 F5.2 s RAs Second of Right Ascension (J2000) 19 A1 --- DE- Declination sign 20- 21 I2 deg DEd Degree of Declination (J2000) 23- 24 I2 arcmin DEm Arcminute of Declination (J2000) 26- 29 F4.1 arcsec DEs Arcsecond of Declination (J2000) 31- 35 F5.2 mag Vmag Averaged V band magnitude 37- 40 F4.2 mag B-V Averaged B-V color index 42- 43 I2 --- N1 Number of WIYN RV measurements 45- 46 I2 --- N2 Number of CfA RV measurements 48- 54 F7.2 km/s RV Mean radial velocity 56- 60 F5.2 km/s e_RV Standard error of RV (1) 62- 67 F6.2 --- e/i ? external/internal error ratio (2) 69- 70 I2 % Mmb ? Calculated RV membership probability 72- 74 A3 --- bin Binarity classification (3) 76- 82 F7.3 km/s gamma ? Center-of-mass radial velocity γ 84-102 A19 --- Com Additional comment
Note (1): If we only have a single measurement, the WIYN or CfA measurement precision is given instead, as appropriate. For binaries with orbital solutions, we provide the error on γ from the orbital fit in this column instead. Note (2): Where "e" is the standard deviation of the RV measurements for the star, and "i" is our measurement precision. Note (3): classifications codes as follows (section 6.3): SM = single member SN = single non-member BM = binary member BN = binary non-member BLM = binary likely member BLN = binary likely non-member BU = binary with unknown membership U = unknown
Global notes: Note (G1): Here, we introduce the WOCS numbering system, based on V magnitude and radial distance from the cluster center. Separate one-dimensional Gaussian fits in right ascension (RA) and declination (DE) to the cluster's apparent density profile (for stars with membership probability p>50%) provides the following new J2000 center 19:41:17.5+40:11:47. Around this center, annuli of 30" width are drawn, and in each ring the stars are sorted in increasing order of their V magnitudes (i.e., the brightest stars have the lowest numbers). If a star is missing a measurement of its V magnitude, it is estimated from the 2MASS catalog using the empirical relationship defined above. The WOCS identification number is the three digit star number followed by the three digit annulus number (e.g., the star 001003 is the brightest star in the third annulus). Sources are identified as <[HGM2009b] WOCS NNNFFF> in Simbad.
History: From electronic version of the journal References: von Hippel et al., Pap I 1998AJ....116.1789V Sarajedini, et al., Pap II 1999AJ....118.2894S Sarajedini, Pap III 1999AJ....118.2321S Barrado y Navascues et al., Pap V 2001ApJ...549..452B Sills & Deliyannis, Pap VI 2000ApJ...544..944S Platais et al., Pap VII 2001AJ....122.1486P, Cat. J/AJ/122/1486 Platais et al., Pap VIII 2002AJ....124..601P, Cat. J/AJ/124/601 Grocholski & Sarajedini,, Pap X 2002AJ....123.1603G von Hippel et al., Pap XI 2002AJ....124.1555V Kafka & Honeycutt, Pap XV 2003AJ....126..276K Grocholski & Sarajedini,, Pap XVI 2003MNRAS.345.1015G Platais et al., Pap XVII 2003AJ....126.2922P, Cat. J/AJ/126/2922 Mathieu et al., Pap XVIII 2004ApJ...602L.121M Sarajedini, et al., Pap XIX 2004AJ....127..991S Kafka et al., Pap XX 2004AJ....127.1622K Hole et al. Pap XXIV 2009AJ....138..159H Platais et al., Pap XXVI 2007A&A...461..509P, Cat. J/A+A/461/509 Geller et al., Pap XXXII 2008AJ....135.2264G, Cat. J/AJ/135/2264 Geller et al., Pap XXXVI 2009AJ....137.3743G, Cat. J/AJ/137/3743 Geller et al., Pap XXXVIII 2010AJ....139.1383G Anthony-Twarog et al., Pap XXXIX 2010AJ....139.2034A
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 15-Nov-2011
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