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J/A+A/545/A12     Chemistry of IRC+10216 inner wind modelled  (Cherchneff, 2012)

The inner wind of IRC+10216 revisited: new exotic chemistry and diagnostic for dust condensation in carbon stars. Cherchneff I. <Astron. Astrophys. 545, A12 (2012)> =2012A&A...545A..12C
ADC_Keywords: Stars, carbon ; Models, evolutionary Keywords: astrochemistry - stars: carbon - stars: AGB and post-AGB - molecular processes Abstract: We model the chemistry of the inner wind of the carbon star IRC+10216 and consider the effects of periodic shocks induced by the stellar pulsation on the gas to follow the non-equilibrium chemistry in the shocked gas layers. We consider a very complete set of chemical families, including hydrocarbons and aromatics, hydrides, halogens, and phosphorous-bearing species. Our derived abundances are compared to those for the latest observational data from large surveys and the Herschel telescope. A semi-analytical formalism based on parameterised fluid equations is used to describe the gas density, velocity, and temperature from 1R to 5R. The chemistry is described using a chemical kinetic network of reactions and a set of stiff, ordinary, coupled differential equations is solved. Description: The following table gives the rates by the Arrhenius expression k=A*(T/300)n*exp(-Ea/T) with A in s-1, cm3/s or cm6/s depending on the type of process, bimolecular, trimolecular, and unimolecular processes, respectively. Objects: ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 09 47 57.2 +13 16 44 IRC +10216 = CW Leo ---------------------------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tablea1.dat 123 378 The chemical reaction network ordered by type of reactions
See also: J/A+A/330/676 : IRC+10216 Silicon and sulfur chemistry (Willacy+ 1998) Byte-by-byte Description of file: tablea1.dat
Bytes Format Units Label Explanations
1 A1 --- Code [ABCD] Code for type of reaction (1) 3- 7 A5 --- Num Reaction number (1) 9- 25 A17 --- React Reactants 27- 28 A2 --- --- [->] 32- 47 A16 --- Prod Products 52- 59 E8.3 --- A A coefficient (in s-1, cm3/s or cm6/s depending on the type of process) 63- 68 F6.2 --- n n factor 72- 78 F7.1 K Ea Activation energy Ea in Kelvin 81-123 A43 --- Ref References for the rate data (2)
Note (1): The chemical reaction network is sub-divided in three categories of processes as follows: A = termolecular (reaction labelled 3B for 3-body) B = collisional/thermal fragmentation (reaction labelled TF for thermal fragmentation) C = neutral-neutral (reaction labelled NN) D = radiative association (reaction labelled RA) Note (2): References as follows: E = estimated rate NIST = National Institute of Standards and Technology Chemical Kinetics Database UDFA06 = UMIST database for Astrochemistry 2006 1 = Andreazza & Singh (1997MNRAS.287..287A) 2 = Andreazza & Marinho (2005ApJ...624.1121A) 3 = Andreazza et al. (2006MNRAS.372.1653A) 4 = Andreazza & Marinho (2007MNRAS.380..365A) 5 = Andreazza et al. (2009MNRAS.400.1892A) 6 = Appleton, Steinberg & Liquornik (1970, J. Chem. Phys., 52, 2205) 7 = Babb & Dalgarno (1995, Phys. Review A 51, 3021) 8 = Cherchneff & Dwek (2010ApJ...713....1C) 9 = Giesen, Herzler & Roth (2003, J. Phys. Chem. A, 107, 5202) 10 = Hanson (1973, J. Chem. Phys., 60, 4970) 11 = Kruse & Roth (1997, J. Phys. Chem. A, 101, 2138) 12 = Miller & Melius (1992, Combustion & Flame 91, 21) 13 = Richter & Howard (2000, Prog. En. Comb. Science 26, 565) 14 = Self & Plane (2003, Phys. Chem. Chem. Phys., 5, 1407) 15 = Singh & Andreazza (2000ApJ...537..261S) 16 = Wakelam et al. (2009A&A...495..513W) 17 = Andreazza et al. (1995ApJ...451..889A) 18 = Scherer (2000, Proceedings of the Combustion Institute 25, 1511) 19 = Woon & Herbst (1996ApJ...465..795W) 20 = Baulch (1992, J. Phys. Chem. Ref. Data 21, 411) 21 = Kumaran (1994, J. Chem. Phys. 101, 9487)
Acknowledgements: Isabelle Cherchneff, isabelle.cherchneff(@)unibas.ch
(End) Patricia Vannier [CDS] 09-Aug-2012
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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