J/AJ/131/414       Structural parameters of SMC star clusters      (Hill+, 2006)

The star clusters of the Small Magellanic Cloud: structural parameters. Hill A., Zaritsky D. <Astron. J., 131, 414-430 (2006)> =2006AJ....131..414H 2006AJ....131..414H (SIMBAD/NED BibCode)
ADC_Keywords: Magellanic Clouds ; Clusters, globular ; Morphology Keywords: galaxies: individual (Small Magellanic Cloud) - galaxies: star clusters - globular clusters: general - Magellanic Clouds Abstract: We present structural parameters for 204 stellar clusters in the Small Magellanic Cloud derived from fitting King and Elson, Fall, and Freeman (EFF, 1987ApJ...323...54E 1987ApJ...323...54E) model profiles to the V-band surface brightness profiles as measured from the Magellanic Clouds Photometric Survey images. Description: The data come from the Magellanic Clouds Photometric Survey (MCPS) described by Zaritsky et al. (2002, Cat. J/AJ/123/855). In summary, we have obtained U, B, V, and I drift-scan images of the central 4.5°x4° area of the SMC using the Las Campanas Swope (1m) telescope and the Great Circle Camera. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 62 204 Cluster designation and position table2.dat 142 204 Structural parameters -------------------------------------------------------------------------------- See also: J/AJ/119/1214 : Census of star clusters in the SMC (Bica+, 2000) J/AJ/123/855 : Magellanic Clouds Photometric Survey: the SMC (Zaritsky+ 2002) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- [RZ2005] Cluster Number 9 I1 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) 22 A1 --- DE- Sign of the Declination (J2000) 23- 24 I2 deg DEd Degree of Declination (J2000) 26- 27 I2 arcmin DEm Arcminute of Declination (J2000) 29- 33 F5.2 arcsec DEs Arcsecond of Declination (J2000) 37- 62 A26 ---- OName Other Cluster Names -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- [RZ2005] Cluster Number 8- 11 F4.2 pc e_CRad Lower 1σ confidence interval on CRad (1) 15- 19 F5.2 pc CRad Best fit King core radius 23- 27 F5.2 pc E_CRad Upper 1σ confidence interval on CRad (1) 31- 35 F5.2 pc e_LRad Lower 1σ confidence interval on LRad (1) 39- 43 F5.2 pc LRad Best fit 90% light radius 47- 51 F5.2 pc E_LRad Upper 1σ confidence interval on LRAd (1) 55- 58 F4.1 mag Vmag King model V-band magnitude (2) 62- 66 I5 ct/arcsec2 Sig King model central count density (2) 70- 73 F4.2 --- Ellip Ellipticity (1-b/a) 78- 81 F4.2 --- chi2 King model Χ2 (2) 85- 89 F5.2 pc e_ERad Lower 1σ confidence interval on ERad (1) 93- 97 F5.2 pc ERad Best fit EFF core radius (4) (3) 101-105 F5.2 pc E_ERad Upper 1σ confidence interval on ERad (1) 109-112 F4.2 --- e_Egam Lower 1σ confidence interval on Egam (1) 116-119 F4.2 --- Egam Best fit γ value 123-126 F4.2 --- E_Egam Upper 1σ confidence interval on Egam (1) 130-134 I5 ct/arcsec2 ESig EFF model central count density (4) 138-142 F5.2 --- Echi2 EFF model Χ2 (4) -------------------------------------------------------------------------------- Note (1): Defined using χ2, and are therefore undefined in the cases where even the best fit model has χ2 greater than the corresponding value for the available degrees of freedom. Note (2): King (1962AJ.....67..471K 1962AJ.....67..471K). Note (3): The core radius, when defined as the radius for which the surface brightness drops to half its central value, can be calculated using rc=a(22/γ-1)0.5. Note (4): Elson, Fall & Freeman (1987ApJ...323...54E 1987ApJ...323...54E). -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Marianne Brouty [CDS] 31-Aug-2006
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