J/A+A/357/572       Dust formation in WC stars    (Cherchneff+, 2000)

Dust formation in carbon-rich Wolf-Rayet stars I. Chemistry of small carbon clusters and silicon species Cherchneff I., Le Teuff Y.H., Williams P.M., Tielens A.G.G.M. <Astron. Astrophys. 357, 572 (2000)> =2000A&A...357..572C 2000A&A...357..572C
ADC_Keywords: Stars, Wolf-Rayet ; Stars, carbon ; Models, evolutionary Keywords: molecular data - molecular processes - stars: circumstellar matter - stars: Wolf-Rayet Description: The following table gives the ratefile of the chemical model. Columns α, β and γ give the rate k at temperature T in the Arrhenius form: k = α * (T/300)β * exp(-γ/T) The arrows indicate reversible reactions. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file tablea.dat 102 407 Reaction data file -------------------------------------------------------------------------------- See also: III/85 : Sixth Catalogue of Galactic Wolf-Rayet Stars (van der Hucht+ 1981) III/136 : Optical spectrophotometry of Wolf-Rayet stars (Torres+ 1987) J/A+A/330/676 : IRC+10216 Silicon and sulfur chemistry (Willacy+ 1998) Byte-by-byte Description of file: tablea.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 5 I4 --- Index Number of reaction 7- 13 A7 --- R1 Reactant 1 15- 21 A7 --- R2 Reactant 2 23- 29 A7 --- R3 Reactant 3 31- 37 A7 --- P1 Product 1 39- 45 A7 --- P2 Product 2 47- 53 A7 --- P3 Product 3 54- 61 E8.2 cm3/s alpha α coefficient (1) 62- 67 F6.2 --- beta β coefficient (1) 68- 76 F9.1 K gamma γ coefficient (1) 78-100 A23 --- Ref Reference (2) -------------------------------------------------------------------------------- Note (1): α is in units of cm6/s for thermolecular reactions (index = 1-27) and in units of s-1 for photo processes (index = 55-108). The rate k at temperature T is k = α * (T/300)β * exp(-γ/T) Note (2): References written in brackets as reactions refer to this reaction. The format has been contracted so that (X Y Z > T U) means: X + Y + Z --> T + U References with an 'E' have an estimated rate, a 'C' a rate calculated from cross sections. References: AH86 = Anicich & Huntress, 1986ApJS...62..553A 1986ApJS...62..553A AS97 = Andreazza & Singh, 1997MNRAS.287..287A 1997MNRAS.287..287A AVG93 = Anicich, 1993ApJS...84..215A 1993ApJS...84..215A Baulch94 = Baulch et al., 1994, J. Phys. Chem. Ref. Data 23, 847 DDY90 = Dalgarno et al., 1990ApJ...349..675D 1990ApJ...349..675D DP79 = Donnelly & Pasternack, 1979, Chem. Phys. 39, 427 FHFM79 = Filseth et al., 1979, Chem. Phys. Lett. 61, 288 MDM77 = Mann, 1977, Chem. Phys. Lett. 47, 106 NIST = Mallard et al., 1994, NIST Chemical Kinetics Database PDAN89 = Petuchowski et al., 1989ApJ...342..406P 1989ApJ...342..406P PST = 1988, Physica Scripta, volume T, 28 R95 = UMIST Database, 1995 version RMW80 = Reisler et al., 1980, Chem. Phys. 47, 49 RW80 = Rakshit & Warneck, 1980, J. Chem. Soc. Farad. II 76, 1084 WC98 = Willacy & Cherchneff, 1998, Cat. J/A+A/330/676 WFB91 = Wlodek et al., 1991, J. Am. Chem. Soc. 113, 4461 -------------------------------------------------------------------------------- Acknowledgements: Yoann Henri Le Teuff
(End) Le Teuff [UMIST], Patricia Bauer [CDS] 11-May-2000
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