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J/A+A/477/165     Nearby open clusters tidal radii and masses  (Piskunov+, 2008)

Tidal radii and masses of open clusters. Piskunov A.E., Schilbach E., Kharchenko N.V., Roeser S., Scholz R.-D. <Astron. Astrophys. 477, 165 (2008)> =2008A&A...477..165P
ADC_Keywords: Clusters, open ; Morphology Keywords: Galaxy: open clusters and associations: general - solar neighbourhood - Galaxy: stellar content Abstract: In a previous paper we obtained King's parameters for 236 of 650 Galactic open clusters identified in the ASCC-2.5 (Kharchenko, 2001, Cat. I/280). Our aims is the estimate tidal radii by use of observable parameters available for all clusters. Bias-free results are required. We use methods of stellar statistics and develop a semi-empirical model of open clusters. Description: The table presents tidal radii and masses of 650 Galactic open clusters. The tidal radii are derived from a relation between a semi-major axis A of the density distributions of cluster members and fitted King radii (J/A+A/468/151). The cluster masses are found from cluster tidal radii assuming that the latter are good approximations of limiting radii for local clusters moving at nearly circular orbits. The clusters are a sample of the Catalogue of Open Cluster Data and their members are selected from the high-precision, homogeneous all-sky catalogue ASCC-2.5 (Kharchenko, 2001, Cat. I/280). The clusters in the table are sorted according to their order in the COCD. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table.dat 124 650 Tidal radii and masses for 650 open clusters
See also: I/280 : All-sky Compiled Cat. of 2.5 million stars (Kharchenko, 2001) J/A+A/438/1163 : Catalogue of Open cluster Data (COCD) (Kharchenko+, 2005) J/A+A/440/403 : 109 new Galactic open clusters (COCD1) (Kharchenko+, 2005) J/A+A/468/151 : Nearby open clusters radii and masses (Piskunov+, 2007) Byte-by-byte Description of file: table.dat
Bytes Format Units Label Explanations
1- 4 I4 --- COCD (1-520, 1001-1130) COCD number 7- 23 A17 --- Name Cluster designation (NGC, IC or other) (1) 25- 31 F7.2 deg GLON Galactic longitude 32- 38 F7.2 deg GLAT Galactic latitude 39- 46 F8.3 mag DistMod Distance modulus 47- 52 F6.2 mag E(B-V) B-V Colour-excess 53- 58 I6 pc Dist Distance 59- 64 F6.2 [yr] logt Logarithm of age 65- 70 F6.1 pc rt ?=-9.9 Tidal radius 71- 76 F6.1 pc e_rt ?=-9.9 rms error rt 77- 85 F9.3 [solMass] logM ?=-9.999 Logarithm of cluster mass 86- 94 F9.3 [solMass] e_logM ?=-9.999 rms error of logM 95-100 F6.1 pc rtA Tidal radius derived from semi-major axis A 101-106 F6.1 pc e_rtA rms error of rtA 107-115 F9.3 [solMass] logMA Log of Cluster mass from semi-major axis A 116-124 F9.3 [solMass] e_logMA rms error of logMA
Note (1): There are clusters which overlap in the plane of the sky some of which also have common members. The most prominent example is the "double cluster" h and chi Per (COCD numbers 29 and 30). Their semi-major axes A are overestimated due to the relatively large number of common members, and so are their individual tidal radii and masses.
Acknowledgements: Ralf-Dieter Scholz, rdscholz(at)aip.de
(End) Patricia Vannier [CDS] 03-Dec-2007
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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