Showing 1 - 20 results of 95 for search '"Crimean Astrophysical Observatory"', query time: 0.53s Refine Results
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    SLITLESS DIGITAL TV SPECTROPHOTOMETER OF THE CRIMEAN ASTROPHYSICAL OBSERVATORY by A. N. Abramenko, N. N. Okhmat, V. V. Prokof'eva, L. M. Sharipova

    Published 2017-11-01
    “…The original slitless spectrograph are created in the Crimean Astrophysical Observatory for 0.5-m meniscus telescope. …”
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    The near-infrared observations at the Tower Solar Telescope TST-2 of the Crimean Astrophysical Observatory by Andreeva Olga, Malashchuk Valentina

    Published 2022-01-01
    “…Observations in the near-infrared wavelength range have been regularly carried out at the Crimean Astrophysical Observatory (CrAO) on the Tower Solar Telescope (TST-2). …”
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    Databases of Publications and Observations as a Part of the Crimean Astronomical Virtual Observatory by Shlyapnikov A., Bondar’ N., Gorbunov M.

    Published 2015-12-01
    “…We describe the main principles of formation of databases (DBs) with information about astronomical objects and their physical characteristics derived from observations obtained at the Crimean Astrophysical Observatory (CrAO) and published in the “Izvestiya of the CrAO” and elsewhere. …”
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    Automatic telescope for observation of near-Earth asteroids by V. V. Rumyantsev, N. S. Chernykh

    Published 2004-12-01
    “…The old 64-cm Richter–Slefogt telescope (F=90 cm) of the Crimean Astrophysical Observatory was reconstructed and equipped with the ST-8 CCD camera supplied by The Planetary Society as the Eugene Shoemaker Near Earth Object Grant. …”
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    HIGH-ACCURACY MAGNETIC FIELD MEASUREMENTS ON COOL GIANT beta GEMINORUM by D. N. Baklanova, S. I. Plachinda

    Published 2010-11-01
    “…We present new high- accuracy magnetic field measurements of β Gem which were obtained during 2010 at Crimean Astrophysical Observatory with 2.6-m telescope and Stokesmeter.…”
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    Asteroids and comets: one-hundredth anniversary of discoveries, observations and researches in Crimea by V. P. Tarashchuk

    Published 2011-12-01
    “…The Second stage – positional, photometric, spectral, polarization works in the Crimean astrophysical observatory for studying the comets and asteroids.…”
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    AM HERCULIS IN 1989-93: VARIOUS TYPES OF PHOTOMETRIC AND POLARIMETRIC BEHAVIOUR by N. M. Shakhovskoy, I. L. Andronov, S. V. Kolesnikov

    Published 2017-07-01
    “…The types of variability of AM Her are discussed on the base of monitoring carried out at the 2.6m Shajn and 1.25cm AZT-11 telescopes of the Crimean Astrophysical observatory. The main types are the following: a) the wavelength-dependent regular variations with the orbital phase more pronounced in RI bands and observed at high and intermediate luminosity states; b) at the low and intermediate states the variations in UB which are usually in antiphase with RI; c) flares caused by the accretion events with colors close to that of the system; d) flares of the secondary of the UV Cet-type.…”
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    Extremely slow nova VI548 Aql by N. Primak, E. P. Pavlenko

    Published 2017-03-01
    “…The results of VRI CCD photomet-rical observations of extremely slow nova V1548 Aql (Nova Aql 2001) in Crimean Astrophysical Observatory during 2001 - 2003 years are presented. …”
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    IS PZ MON A RED DWARF OR A RED GIANT? by N. I. Bondar', S. G. Sergeev

    Published 2016-12-01
    “…There are presented spectra of PZ Mon in the region 3750-6150 Α with resolution of 7 ≈ Α, which were carried out in the Nasmith focus of 2.6 m reflector in the Crimean Astrophysical observatory. Intensities of molecular absorptions in this spectral range are determined relative a nearby continuum and their relations between absolute magnitudes are considered. …”
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    Determining the size of craters on the surfaces of atmosphereless bodies in Solar system with ground-based methods by A. I. Klianchin, V. V. Prokof'eva-Mikchailovskaya

    Published 2013-12-01
    “…A new method of determining the size of craters on the surfaces of atmosphereless bodies of the Solar system, called spectral-frequency method (SFM), was developed at the Crimean Astrophysical Observatory by V. V. Prokofieva-Mikhaylovska, N. …”
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