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: http://www.inasan.rssi.ru/~shematov/Astrochemistry_2004.html
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On
the master equation approach to diffusive grain-surface chemistry: The H, O, CO
system.
Astronomy and Astrophysics, 2002, 391, 1069.
Deuterium
fractionation on interstellar grains studied with modified rate equations and a
Planetary
and Space Science, 2002, 50, 1267-1266.
New approaches to the modeling of surface chemistry on the interstellar
grains.
Astrophysics and Space Science, 2003, 285, 725-735.
Chemical and dynamical evolution
of protostellar clouds: initial stages of collapse (abstract).
Astronomy Reports, 1996, 40, 639-652 [AZh, 73, 702-716],
Self-consistent model of chemical and dynamical evolution of protostellar clouds.
MNRAS, 1997, 292, 601-610 ( preprint).
Chemical
and dynamical evolution of protostellar clouds:
chemistry at early stages of collapse (abstract).
Astronomy Reports, 1999, 43, 645-656 [AZh, 76, 738-750].
- Chemical and dynamical models of starless
cores:
A Coupled Dynamical and Chemical Model of Starless Cores of Magnetized
Molecular Clouds.
I. Formulation and Initial Results.
Astrophys. J., 2002, 569,792-801.
A Coupled Dynamical and Chemical Model of Starless Cores of Magnetized
Molecular Clouds.
II. Chemical Differentiation.
Astrophys. J., 2003, 588, 894-909.
A
coupled dynamical and chemical model for starless core L1544: Comparison of
modeled and observed
C18O, HCO+ and CS emission spectra. (abstract).
Astronomy
Reports,
2003, 47, 176-185 [AZh, 80, 202-211].
Chemical Differentiation in Strongly Magnetized Starless Cores.
SFChem 2002:
Chemistry as a Diagnostic of Star Formation, proceedings of a conference held
at
To be published by NRC Press,