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 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 1997MNRAS.287..287A) 2 = Andreazza & Marinho (2005ApJ...624.1121A 2005ApJ...624.1121A) 3 = Andreazza et al. (2006MNRAS.372.1653A 2006MNRAS.372.1653A) 4 = Andreazza & Marinho (2007MNRAS.380..365A 2007MNRAS.380..365A) 5 = Andreazza et al. (2009MNRAS.400.1892A 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 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 2000ApJ...537..261S) 16 = Wakelam et al. (2009A&A...495..513W 2009A&A...495..513W) 17 = Andreazza et al. (1995ApJ...451..889A 1995ApJ...451..889A) 18 = Scherer (2000, Proceedings of the Combustion Institute 25, 1511) 19 = Woon & Herbst (1996ApJ...465..795W 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