Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://www.inasan.rssi.ru/~shematov/Astrochemistry_2004.html
Äàòà èçìåíåíèÿ: Mon Oct 16 16:03:24 2006
Äàòà èíäåêñèðîâàíèÿ: Wed Jan 30 01:21:04 2013
Êîäèðîâêà:
Ïîèñêîâûå ñëîâà: ï ï ï ï ï ï ï ï ï ï ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ð ï ï ï ï ï ï ï ï ï ï
dsmc

ASTROCHEMISTRY OF MOLECULAR CLOUDS:

 

- Stochastic astrochemical kinetics:

  • Stantcheva, T., Shematovich, V.I., and Herbst, E.

      On the master equation approach to diffusive grain-surface chemistry: The H, O, CO system.

      Astronomy and Astrophysics, 2002, 391, 1069.

  • Caselli, P., Stantcheva, T., Shalabiea, O., Shematovich, V.I., and Herbst, E.

      Deuterium fractionation on interstellar grains studied with modified rate equations and a Monte Carlo approach.

      Planetary and Space Science, 2002, 50, 1267-1266.

  • Herbst, E., and Shematovich, V.I.

     New approaches to the modeling of surface chemistry on the interstellar grains.

          Astrophysics and Space Science, 2003, 285, 725-735.

 

- Self-consistent simulation of chemical and dynamical evolution of protostellar clouds:

  • Wiebe D.S., Shematovich V.I., and Shustov B.M.

      Chemical and dynamical evolution of protostellar clouds: initial stages of collapse (abstract).

      Astronomy Reports, 1996, 40, 639-652 [AZh, 73, 702-716],

  • Shematovich V. I , Shustov B. M., and Wiebe D. S.

      Self-consistent model of chemical and dynamical evolution of protostellar clouds.

      MNRAS, 1997, 292, 601-610 ( preprint).

  • Shematovich V.I., Wiebe D.S., and Shustov B.M.

     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:

  • Li, Z.-Y., Shematovich, V. I., Wiebe, D. S., and Shustov, B. M.

     A Coupled Dynamical and Chemical Model of Starless Cores of Magnetized Molecular Clouds.

     I. Formulation and Initial Results.

     Astrophys. J., 2002, 569,792-801.

  • Shematovich, V. I., Wiebe, D. S., Shustov, B. M., and Li, Z.-Y.

      A Coupled Dynamical and Chemical Model of Starless Cores of Magnetized Molecular Clouds.

     II. Chemical Differentiation.

     Astrophys. J., 2003, 588, 894-909.

  • Pavlyuchenkov Ya.N.,Shustov B.M., Shematovich V.I., Wiebe D.S., and Li Z.-Y.

      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].

  • Shematovich V.I., Shustov B.M., Wiebe D.S., Pavlyuchenkov Ya.N., and Li Z.-Y.

      Chemical Differentiation in Strongly Magnetized Starless Cores.

      SFChem 2002: Chemistry as a Diagnostic of Star Formation, proceedings of a conference held August 21-23, 2002

      at University of Waterloo, Waterloo, Ontario, Canada N2L 3G1. Edited by Charles L. Curry and Michel Fich.

      To be published by NRC Press, Ottawa, Canada, p. 101.