Multilayer modeling of porous grain surface chemistry - I. The GRAINOBLE model

作者: V. Taquet , C. Ceccarelli , C. Kahane

DOI: 10.1051/0004-6361/201117802

关键词:

摘要: Context. Mantles of iced water mixed with carbon monoxyde, formaldehyde, and methanol are formed during the so-called prestellar core phase. In addition, radicals also thought to be on grain surfaces, react form complex organic molecules later on, warm-up phase protostellar evolution. Aims. We aim study formation mantles abundance methanol, trapped in them. Methods. have developed a macrosopic statistic multilayer model that follows time includes two effects may increase number mantles: i) mantle formation, only surface layer is chemically active not entire bulk; ii) porous structure grains allows trapping reactive particles. The considers network H, O, CO forming neutral species such as water, CO, plus several radicals. ran large grid models impact nature structure. we explored how uncertainty other key parameters influences composition. Results. Our predicts relatively high abundances radicals, especially HCO CH3 O( 10 −9 −10 −7 ). approach enables us follow chemical differentiation within mantle, showing far from being uniform. For example, mostly present outer layers mantles, whereas inner layers. overall composition depends density age well some microscopic parameters, diffusion energy hydrogenation reactions activation energy. Comparison observations constrain value last (0.5–0.65 1500 K, respectively) provide indications physical conditions ices.

参考文章(112)
G. D. Parfitt, M. J. Jaycock, Chemistry of Interfaces ,(1980)
A. Bacmann, S. Guieu, J. Steinacker, L. Pagani, Direct evidence of dust growth in L183 from MIR light scattering arXiv: Astrophysics of Galaxies. ,(2009) , 10.1051/0004-6361/200912835
M. Ikeda, M. Ohishi, A. Nummelin, J. E. Dickens, P. Bergman, A. Hjalmarson, W. M. Irvine, Survey observations of c-C2H4O and CH3CHO toward massive star-forming regions The Astrophysical Journal. ,vol. 560, pp. 792- 805 ,(2001) , 10.1086/322957
M. A. Requena-Torres, J. Martín-Pintado, A. Rodríguez-Franco, S. Martín, N. J. Rodríguez-Fernández, P. de Vicente, Organic Molecules in the Galactic Center. Hot Core Chemistry without Hot Cores Astronomy and Astrophysics. ,vol. 455, pp. 971- 985 ,(2006) , 10.1051/0004-6361:20065190
M.P. Collings, J.W. Dever, H.J. Fraser, M.R.S. McCoustra, Laboratory studies of the interaction of carbon monoxide with water ice Astrophysics and Space Science. ,vol. 285, pp. 633- 659 ,(2003) , 10.1023/A:1026144806831
Zainab Awad, Serena Viti, Mark P. Collings, David A. Williams, Warm cores around regions of low-mass star formation Monthly Notices of the Royal Astronomical Society. ,vol. 407, pp. 2511- 2518 ,(2010) , 10.1111/J.1365-2966.2010.17077.X
Carlos Sosa, H. Bernhard Schlegel, Ab initio calculations on the barrier height for the hydrogen addition to ethylene and formaldehyde. The importance of spin projection International Journal of Quantum Chemistry. ,vol. 29, pp. 1001- 1015 ,(1986) , 10.1002/QUA.560290435
J. S. Mathis, W. Rumpl, K. H. Nordsieck, The size distribution of interstellar grains The Astrophysical Journal. ,vol. 217, pp. 425- 433 ,(1977) , 10.1086/155591
R. T. Garrod, E. Herbst, Formation of methyl formate and other organic species in the warm-up phase of hot molecular cores Astronomy and Astrophysics. ,vol. 457, pp. 927- 936 ,(2006) , 10.1051/0004-6361:20065560
Hendrik Ulbricht, Gunnar Moos, Tobias Hertel, Physisorption of molecular oxygen on single-wall carbon nanotube bundles and graphite Physical Review B. ,vol. 66, pp. 075404-1- 075404-7 ,(2002) , 10.1103/PHYSREVB.66.075404