Magnetic Flux Loss from Interstellar Clouds with Various Grain Size Distributions
نویسندگان
چکیده
منابع مشابه
Efficient simulations of gas-grain chemistry in interstellar clouds.
Chemical reactions on dust grains are of crucial importance in interstellar chemistry because they produce molecular hydrogen and various organic molecules. Because of the submicron size of the grains and the low flux, the surface populations of reactive species are small and strongly fluctuate. Under these conditions rate equations fail and the master equation is needed for modeling these reac...
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E. Martínez,1,* P. Mikheenko,2,† M. Martínez-López,1 A. Millán,1 A. Bevan,2 and J. S. Abell2 1Instituto de Ciencia de Materiales de Aragón, CSIC–Universidad de Zaragoza, C/María de Luna 3, 50018 Zaragoza, Spain 2Metallurgy and Materials, School of Engineering, University of Birmingham, Edgbaston, Birmingham B15 2TT, United Kingdom Received 31 October 2006; revised manuscript received 21 Decembe...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1990
ISSN: 0074-1809
DOI: 10.1017/s0074180900190217