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Дата изменения: Unknown
Дата индексирования: Mon Apr 11 04:51:21 2016
Кодировка: koi8-r
Поисковые слова: dra
Activity - Page 3

  • Gusev A.S., Kharchenko N.V., Sakhibov F. Kh., et al.A spectral and photometric study of 102 star forming regions in seven spiral galaxies. 2016,MNRAS, 2016MNRAS.tmp....9G
  • Ségransan D., Martín E. L., Lazorenko P.F., et al.Parallax of the L4.5 dwarf 2M1821+ 14 from high- precision astrometry with OSIRIS at GTC. 2016,MNRAS,Vol.455,is.1,p.357-369. 2016MNRAS.455..357S
  • Evans A., Pavlenko Ya.V., Kaminsky B.M., et al.Modelling the spectral energy distribution of the red giant in RS Ophiuchi: evidence for irradiation. 2016,MNRAS,Vol.456,is.1,p.181-191. 2016MNRAS.456..181P
  • Začs L., Pavlenko Ya.V., Kaminsky B.M., et al.Spectroscopic Variability of IRAS 22272+ 5435. 2016,ApJ,Vol.816,is.1,p.3. 2016ApJ...816....3Z
  • Southworth, John, Tregloan-Reed J., Elyiv A.A.,High- precision photometry by telescope defocussing. VIII. WASP- 22, WASP-41, WASP- 42 and WASP- 55. 2016,MNRAS, 2016MNRAS.tmp...77S
  • Mancini L., Ciceri S., Elyiv A.A.,Physical properties of the planetary systems WASP- 45 and WASP- 46 from simultaneous multiband photometry. 2016,MNRAS,Vol.456,Is.1,p.990-1002. 2016MNRAS.456..990C

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The Department for Physics of Stars and Galaxies - Activity

Page 3 of 5

MAIN AREAS OF RESEARCH

  • Determination of baryonic matter in the universe and cosmological nucleosynthesis deviations from the standard model.
  • Investigation of physical characteristics and evolution of galaxies with active star formation, according to observations at telescopes in the world's largest X-ray, ultraviolet, visible, infrared and radio wavelengths of electromagnetic radiation.
  • Development of methods for determining the physical and chemical composition of extragalactic HII regions.
  • The study of the chemical evolution of galaxies.
  • Determination of kinematic and physical characteristics of galaxy clusters.
  • The analysis of stellar spectra considering deviations from LTE, the evolution and definition of the physical characteristics of stars of late spectral classes..