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Перегляд Кинематика и физика небесных тел, 2005, № 5-додаток за назвою

Репозиторій DSpace/Manakin

Перегляд Кинематика и физика небесных тел, 2005, № 5-додаток за назвою

Сортувати за: Порядок: Результатів:

  • Ultracool dwarfs 
    Pavlenko, Ya.V. (Кинематика и физика небесных тел, 2005)
    We present results of modelling of spectra of M-, L-, T-dwarfs. Theoretical spectra are fitted to observed spectra to study the main parameters of the low-mass objects beyond the bottom of the Main Sequence. Application ...
  • Variations of the energy spectra of solar X-ray flares: interconnection with the photospheric, chromospheric, and magnetic activity of the Sun (1972−2001) 
    Kasinskii, V. (Кинематика и физика небесных тел, 2005)
    The problem of flare energy distribution of the Sun is strongly related to the power-law energy spectra of flares on the UV Ceti-type stars. In a preliminary study (1972–1993), the X-ray flare integral energy spectrum (IES) ...
  • Variations of the quasar radio spectra with period 130 h⁻¹ Mpc 
    Khodyachikh, M. (Кинематика и физика небесных тел, 2005)
    It is known that the spatial distribution of galaxies and quasars is structured at a scale LS = 130 h⁻¹Mpc. The same scale can be present at a spatial distribution of the physical characteristics of quasars. The search of ...
  • What limits the precision of ground-based stellar photometry and positional measurements? 
    Zhilyaev, B.E.; Romanyuk, Ya.O.; Verlyuk, I.A.; Svyatogorov, O.A.; Lovkaya, M.N. (Кинематика и физика небесных тел, 2005)
    Nobody has reached the photometric precision better than 0.001 of a magnitude with ground-based telescopes. At the same time, we should spend barely some seconds of time to detect a million photons from any bright star and ...
  • Winds of Wolf−Rayet stars: phenomenology of mass loss 
    Marchenko, S.V. (Кинематика и физика небесных тел, 2005)
    Population I Wolf–Rayet (WR) stars are the evolved descendants of massive (M ≥ 25M) O-type stars. The dense, fast radiatively-drivenWR winds efficiently hide all vital information about basic characteristics of the stellar ...
  • β Lyrae: on the magnetic field 
    Skulsky, M.; Plachinda, S. (Кинематика и физика небесных тел, 2005)
    β Lyrae shows a complicated and intricate time-dependent behaviour of the magnetic field.

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