J/A+A/453/923       Morphologies in the Cepheus Flare region       (Kiss+, 2006)

Star formation in the Cepheus Flare region - Implications from morphology and infrared properties of optically selected clouds. Kiss Z.T., Toth L.V., Krause O., Kun M, Stickel M. <Astron. Astrophys. 453, 923 (2006)> =2006A&A...453..923K 2006A&A...453..923K
ADC_Keywords: Molecular clouds ; Interstellar medium ; Extinction ; Morphology Keywords: ISM: clouds - dust, extinction - ISM: structure - stars: formation - Galaxy: solar neighbourhood - infrared: ISM Abstract: These tables contain the data of the cloud sample on which the study of the relationships between cloud morphology, optical and IR properties, and star formation is based. The sample was defined using the extinction map of the Cepheus Flare region covering ∼256 square degrees created from the B band star counts of the USNO-A2.0 catalogue (Cat. I/252) with a typical resolution of 3 arcminutes on a 1.5 arcminute grid. Cloud definition and description was carried out using automatized methods. The main table lists the positions, peak extinctions, sizes, morphological parameters and classes, distances, mass estimations, parent cloud complexes, and the number of YSO candidates associated. An additional table with the names of the previously catalogued associated clouds and their references is also available. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea1.dat 119 208 Main table tablea2.dat 269 208 Table of associated clouds notes.dat 82 25 References for Simbad names -------------------------------------------------------------------------------- See also: I/252 : The USNO-A2.0 Catalogue (Monet+ 1998) II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003) Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Seq Sequential number of cloud 5- 15 A11 --- Name Name of the cloud 17- 22 F6.2 deg GLON Galactic longitude 24- 29 F6.2 deg GLAT Galactic latitude 31- 33 F3.1 mag AVU Peak extinction from optical (USNO) data 35- 38 F4.1 mag AV2M Peak extinction from NIR (2MASS) data 40- 43 F4.1 K TDC ? Minimum 100-170um dust colour temperature 45- 48 F4.1 arcmin aa Apparent length of major axis 50- 53 F4.1 pc al Linear length of major axis 55- 57 F3.1 --- b/a Apparent axis ratio 59- 61 I3 deg PA *Position angle 63- 66 F4.1 arcmin Dp Peak displacement (distance to cloud center) 68- 70 I3 deg DPA *Displacement direction angle 72- 75 F4.2 --- Sym *Symmetry parameter 77- 80 F4.2 --- Sep *Separateness parameter 82- 85 F4.2 --- Irr *Irregularity parameter 87- 90 A4 --- Class *Morphlogical class 92- 94 I3 pc D1 *Distance of the first component 96- 98 I3 pc D2 *? Distance of the second component 100-102 I3 pc D3 *? Distance of the third component 104-107 I4 solMass Mass Mass from extinction 109-114 A6 --- Ncmpl *Complex name 116-117 I2 --- NYSO *? Number of YSO candidates associated 119 A1 --- Loop *[L] Loop flag -------------------------------------------------------------------------------- Note on PA: In the range of 0-180 deg ccw from the direction of the northern galactic pole. Note on DPA: In the range of 0-180 deg ccw from the direction of the major axis. Note on Sym: The ratio of the sums of extinction in the two halves of the cloud separated by the minor axis Note on Sep: Ratio of the sum of extinction in the defined ellipse, to the sum of extinction in the elliptical ring between this ellipse and that enlarged by a factor of 1.41. Note on Irr: Ratio of the cloud area inside the boundaries, but outside the ellipse defined, to the total area of the cloud. Note on Class: Morphological classes: head-tail (h-t), globular (glob) Note on D1, D2, D3: Adopted distance values as follows: 177 = 200±20pc, Kun, 1998, Cat. J/ApJS/115/59 265 = 288±25pc, Straizys, 1992BaltA...1..149S 1992BaltA...1..149S 277 = 300±30pc, Kun, 1998, Cat. J/ApJS/115/59 302 = 325±13pc, Straizys, 1992BaltA...1..149S 1992BaltA...1..149S 377 = 400±80pc, Racine, 1968AJ.....73..233R 1968AJ.....73..233R 427 = 450±100pc, Kun, 1998, Cat. J/ApJS/115/59 627 = 650±70pc, Racine,1968AJ.....73..233R 1968AJ.....73..233R 877 = 900±100pc, Kun, 1998, Cat. J/ApJS/115/59 Note on Ncmpl: Complexes are also defined in the paper. Note on NYSO: Young IRAS sources, H alpha stars, and T Tauri like 2MASS sources were considered. Note on Loop: Clouds marked with L are situated on the shell of an infrared loop of Kiss et al. (2004, Cat. J/A+A/418/131). -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 3 I3 --- Seq Sequential number of cloud 5- 15 A11 --- Name Name of the cloud 17- 22 F6.2 deg GLON Galactic longitude 24- 29 F6.2 deg GLAT Galactic latitude 31-269 A239 --- List List of associated cloud names (1) -------------------------------------------------------------------------------- Note (1): The references are in notes.dat file. -------------------------------------------------------------------------------- Byte-by-byte Description of file: notes.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Name Simbad acronym 12- 30 A19 --- BibCode BibCode 32- 55 A24 --- Aut Author's name 62- 82 A21 --- Com Comments -------------------------------------------------------------------------------- Nomenclature note: In the abstract of the paper, object GIRL G109+11 corresponds to GIRL G109+10 in Kiss et al., 2004, Cat. J/A+A/418/131. Acknowledgements: Zoltan Kiss, kissz(at)alcyone.bajaobs.hu
(End) Zoltan Tamas Kiss [Baja Astron. Obs.], Patricia Vannier [CDS] 07-Apr-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