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Literatura

1. Ward-Thompson D. Isolated star formation: from cloud formation to core collapse // Science. 2002. Vol. 295. P. 76.

2. Hartmann L., Ballesteros-Paredes J., Bergin E. A. Rapid formation of molecular clouds and stars in the solar neighborhood // Astrophys. J. 2001. Vol. 562. P. 852.

3. Pringle J. E., Allen R. J., Lubow S. H. The formation of molecular clouds // Mon. Not. Roy. Astron. Soc. 2001. Vol. 327. P. 663.

4. Ohishi M., Irvine W. M., Kaifu N. Molecular abundance variations among and within cold, dark molecular clouds // Astrochemistry of Cosmic Phenomena. Ed. P. D. Singh. Dordrecht: Kluwer, 1992. P.171.

5. Herbst E., Klemperer W. The formation and depletion of molecules in dense interstellar clouds // Astrophys. J. 1973. Vol. 185. P. 505.

6. Tafalla M., Myers P. C., Caselli P. et all Systematic molecular differentiation in starless cores // Astrophys. J. 2002. Vol. 569. P. 815.

7. van Dishoeck E. F., Blake G. A. Chemical evolution of star-forming regions // Ann. Rev. Astron. Astrophys. 1998. Vol. 36. P. 317.

8. Millar T. J., Farquhar P. R. A., Willacy K. The UMIST Database for Astrochemistry 1995 // Astron. Astrophys. Sup. 1997. Vol. 121. P. 139.

9. Terzieva R., Herbst E. The sensitivity of gas-phase chemical models of interstellar clouds to C and O elemental abundances and to a new formation mechanism for ammonia // Astrophys. J. 1998. Vol. 501. P. 207.

10. Snell R. L., Howe J. E., Ashby M. L. N. et al. Water abundance in molecular cloud cores // Astrophys. J. Lett. 2000. Vol. 539. P. L101.

11. Hasegawa T. I., Herbst E., Leung C. M. Models of gas-grain chemistry in dense interstellar clouds with complex organic molecules // Astrophys. J. Sup. 1992. Vol. 82. P. 167.

12. Anders E., Grevesse N. Abundances of the elements: meteoritic and solar // Geochim. Cosmochim. Acta. 1989. Vol. 53. P. 197.

13. Grevesse N., Sauval A. J. Standard solar composition // Space Science Rev. 1998. Vol. 85. P. 161.

14. Aikawa Y., Herbst E. Deuterium fractionation in protoplanetary disks // Astrophys. J. 1999. Vol. 526. P. 314.

15. Bergin E. A., Langer W. D., Goldsmith P. F. Gas-phase chemistry in dense interstellar clouds including grain surface molecular depletion and desorption // Ibid. 1995. Vol. 441. P. 222.

16. Shalabeia O. M. The effect of the initial elemental abundance on gas-grain chemical models // Astron. Astrophys. 2001. Vol. 370. P. 1044.

17. Bergin E. A., Langer W. D. Chemical evolution in preprotostellar and protostellar cores // Astrophys. J. 1997. Vol. 486. P. 316.

18. Aikawa, Y., Ohashi, N., Inutsuka, S. et all Molecular evolution in collapsing prestellar cores // Astrophys. J. 2001. Vol. 552. P. 639.

19. Shematovich V. I., Shustov B. M. , Wiebe D. S. Self-consistent model of chemical and dynamical evolution of protostellar clouds // Mon. Not. Roy. Astron. Soc. 1997. Vol. 292. P. 601.

20. Li Z.-Y., Shematovich V. I., Wiebe D. S. et all A coupled dynamic and chemical model of starless cores of magnetized molecular clouds. I. Formulation and initial results // Astrophys. J. 2002. Vol. 569. P. 792.

21. Evans N. J. II Physical conditions in regions of star formation // Ann. Rev. Astron. Astrophys. 1999. Vol. 37. P. 311.

22. Pavlyuchenkov Ya. N., Shustov B. M., Shematovich V. I. i dr. Himiko-dinamicheskaya model' dozvezdnogo yadra L1544: sravnenie model'nyh i nablyudaemyh spektrov izlucheniya CO, HCO i CS // Astronom. zhurn. 2003. (V pechati).

23. Roberts H., Herbst E. The abundance of gaseous HO and O in cores of dense interstellar clouds // Astron. Astrophys. 2002. Vol. 395. P. 233.

24. Wiebe D., Semenov D., Henning Th. Reduction of chemical networks. I. The case of molecular clouds // Ibid. 2003. (In press).



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