J/ApJ/611/270     Magellanic star clusters IR fluctuations     (Gonzalez+, 2004)

Infrared surface brightness fluctuations of Magellanic star clusters. Gonzalez R.A., Liu M.C., Bruzual A.G. <Astrophys. J., 611, 270-293 (2004)> =2004ApJ...611..270G 2004ApJ...611..270G
ADC_Keywords: Associations, stellar ; Magellanic Clouds ; Stars, giant Keywords: astronomical data bases: miscellaneous - galaxies: distances and redshifts - galaxies: star clusters - Magellanic Clouds - stars: AGB and post-AGB Abstract: We present surface brightness fluctuations (SBFs) in the near-IR for 191 Magellanic star clusters available in the Second Incremental and All Sky Data releases of the Two Micron All Sky Survey (2MASS, Cat. II/246) and compare them with SBFs of Fornax Cluster galaxies and with predictions from stellar population models as well. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 72 191 Cluster data -------------------------------------------------------------------------------- See also: II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- SCl Supercluster type (co-added clusters of same SWB class) 10- 15 E6.2 yr Age Cohen (1982ApJ...258..143C 1982ApJ...258..143C) supercluster age (1) 17- 22 F6.4 --- Z Cohen (1982ApJ...258..143C 1982ApJ...258..143C) supercluster metallicity 24- 27 A4 arcsec --- [0-60-] Limiting radii of analyzed region (2) 29- 46 A18 --- Name Star cluster name 48- 49 A2 --- Orig Origin of the data Name (3) 51- 52 I2 --- Num Number of 2MASS PSC stars in analysis 54- 55 I2 --- sPar Elson & Fall (1985ApJ...299..211E 1985ApJ...299..211E; 1988AJ.....96.1383E 1988AJ.....96.1383E) s-parameter (related to the age) 57- 59 A3 --- Cloud Cloud name star cluster belongs to 61- 64 F4.2 mag E(B-V) ? Persson et al. (1983ApJ...266..105P 1983ApJ...266..105P) E(B-V) (4) 66- 71 A6 --- SWB Cluster SWB class (5) -------------------------------------------------------------------------------- Note (1): For the Pre-SWB supercluster only, we have adopted the age of a cluster with s=7 from Elson & Fall (1985ApJ...299..211E 1985ApJ...299..211E). Note (2): In arcseconds at the distance of the LMC. Note (3): Origin of the data, defined as follows: a = Data from All Sky Data Release of 2MASS (Cat. II/246); b = Clusters added to sample from Elson & Fall (1988AJ.....96.1383E 1988AJ.....96.1383E); c = Listed as IC 1665 in both van den Bergh (1981A&AS...46...79V 1981A&AS...46...79V) and Elson & Fall (1985ApJ...299..211E 1985ApJ...299..211E). Note (4): Otherwise, we have assumed E(B-V)=0.075, and E(B-V)=0.037 for the SMC (Schlegel, Finkbeiner, & Davis 1998ApJ...500..525S 1998ApJ...500..525S). Note (5): SWB classification from Searle, Wilkinson and Bagnuolo (1980ApJ...239..803S 1980ApJ...239..803S), which constitutes a smooth, one-dimensional sequence of increasing age and decreasing metallicity from from pre-SWB (very young) to SWB-VII -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 13-Oct-2005
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