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Methanol formation: A Monte Carlo study

Published online by Cambridge University Press:  01 February 2008

Ankan Das ,
Kinsuk Acharyya ,
Sonali Chakrabarti  and
Sandip K. Chakrabarti
Ankan Das
Affiliation:
Indian Centre for Space Physics, Chalantika 43, Garia Station Road, Kolkata 700084, India email: [email protected]
Kinsuk Acharyya
Affiliation:
S. N. Bose National Centre for Basic SciencesSalt Lake, Kolkata 700098, India email: [email protected], [email protected]
Sonali Chakrabarti
Affiliation:
Indian Centre for Space Physics, Chalantika 43, Garia Station Road, Kolkata 700084, India email: [email protected] Maharaja Manindra Chandra College20 Ramakanta Bose Lane, Kolkata 700003, India email: [email protected]
Sandip K. Chakrabarti
Affiliation:
Indian Centre for Space Physics, Chalantika 43, Garia Station Road, Kolkata 700084, India email: [email protected] S. N. Bose National Centre for Basic SciencesSalt Lake, Kolkata 700098, India email: [email protected], [email protected]
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Abstract

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We carry out a Monte-Carlo simulation to study the formation of methanol on the grain surfaces. We found that the recombination efficiencies are strongly dependent on the extrinsic properties of the grain, such as the number of sites on the grain surface and the flux of the accreting matter. This uses the concept of effective grain surface (denoted through a factor α) area which changes as the grain is populated.

Keywords

ISM: abundancesISM: moleculesmethods: numericalmolecular processes
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S251: Organic Matter in Space , February 2008 , pp. 121 - 122
Copyright
Copyright © International Astronomical Union 2008

References

Acharyya, K., Chakrabarti, S. K., & Chakrabarti, S. 2005, MNRAS, 361, 550CrossRefGoogle Scholar
Chakrabarti, S. K., Das, A., Acharyya, K., & Chakrabarti, S. 2006a, A&A, 457, 167Google Scholar
Chakrabarti, S. K., Das, A., Acharyya, K., & Chakrabarti, S. 2006b, BASI, 34, 299Google Scholar
Gibb, E. L., et al. 2000, ApJ, 536, 347CrossRefGoogle Scholar
Hasegawa, T., Herbst, E., & Leung, C. M. 1992, ApJS, 82, 167CrossRefGoogle Scholar
Roberts, H. & Herbst, E. 2002, A&A, 395, 233Google Scholar