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Astronomical Research and Education in Tajikistan

Published online by Cambridge University Press:  25 April 2016

Pulat B. Babadzhanov
Pulat B. Babadzhanov*
Affiliation:
Institute of Astrophysics, Dushanbe 734042, Tajikistan. e-mail: [email protected]

Abstract

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Astronomical researches in Tajikistan are carried out by the Institute of Astrophysics, Tajik Academy of Sciences. The main scientific fields of investigation are physics and dynamics of asteroids, comets and meteors, variable stars and observations of artificial Earth satellites. The Institute has three observational stations: the Gissar observatory (at an altitude 730 m above sea-level) with photographic fireball and meteor patrols, a 70-cm reflector, a 40-cm Zeiss astrograph, a high-precision astronomical telescope (D=1 m, F=0.75 m), etc.; the Sanglokh observatory (at an altitude 2300 m above sea-level) with a Ritchey-Chretien 1-m telescope and 0.6-m reflector by Carl Zeiss; the Pamir observatory (at an altitude 4350 m above sea-level) with a 70-cm reflector. In 1999 the Department of Astronomy was restored in the Tajik State National University and the first students were admitted to this university for the astronomical profession.

Type
Section 4: Current Status of Astronomy Research in Developing Countries
Information
Transactions of the International Astronomical Union , Volume 24 , Issue 3: Special session: Astronomy for Developing Countries , 2001 , pp. 187 - 196
Copyright
Copyright © Astronomical Society of Pacific 2001

References

Babadzhanov, P.B. 1994, Asteroids, Comets, Meteors 1993, 45–54.Google Scholar
Babadzhanov, P.B. 1998, Cel.Mech. & Dynam.Astronomy, 69, p. 221.CrossRefGoogle Scholar
Babadzhanov, P.B., Bibarsov, R.Sh., & Kolmakov, V.M. 1990, Mass Distribution and the Flux of Sporadic Meteoroids, Moscow, 56 pp.Google Scholar
Babadzhanov, P.B., Kashcheyev, B.L., Nechitaylenko, V.A., & Fedynskiy, V.V. 1974, Radar-meteor investigation of the high-atmosphere circulation, Publishing house “Donish”, Dushanbe, 172 pp.Google Scholar
Borisov, Yu.V. & Minikulov, N.K. 1997, Bull. Inst. Astrophys., Tajik Acad.Sci., No 83 , p.19.Google Scholar
Borisov, Yu.B. & Redkina, N.P. 1997, Bull. Inst. Astrophys., Tajik Academy of Sci., No 83 , p. 3.Google Scholar
Dobrovolsky, O.V. 1966, Comets, Moscow, Nauka, 288 pp.Google Scholar
Ibadinov, Kh.I. 1993, Doklady Academii nauk Resp. Tajikistan, XXXVI, No 3 , p.182.Google Scholar
Ibadov, S. 1996, Physical Processes in Comets and Related Objects, Moscow, Kosmoinform Publ. Comp., 181 pp.Google Scholar
Kanaev, I.I., Sholomitsky, G.B., Maslov, LA., & Grozdilov, V.M. 1983, Review of Science and Technics (Series of “Astronomy”), Vol. 22, p. 286.Google Scholar
Kiselev, N.N., Minikulov, N.K., & Chernova, G.P. 1995, Bull. Inst. Astrophys., Tajik Acad. Sci., No 82, p. 42.Google Scholar
Redkina, N.P. & Zausaeva, O.G. 1997, Bull. Inst. Astrophys, Tajik Acad. Sci., No 83 , p. 7.Google Scholar
Shevchenko, V.S. 1972, Young Star Complexes. Astroclimat, Publ, house “Fan”, Uzbekistan, p. 84.Google Scholar