A spectroscopic study of the peculiar galaxy UGC 5600     

L. V. Shalyapina  A. V. Moiseev  V. A. Yakovleva 《Astronomy Letters》2002,28(7):443-453

We present our observations of the galaxy UGS 5600 with a long-slit spectrograph (UAGS) and a multipupil field spectrograph (MPFS) attached to the 6-m Special Astrophysical Observatory telescope. Radial-velocity fields of the stellar and gaseous components were constructed for the central region and inner ring of the galaxy. We proved the existence of two nearly orthogonal kinematic subsystems and conclude that UGC 5600 is a galaxy with an inner polar ring. In the circumnuclear region, we detected noncircular stellar motions and suspected the existence of a minibar. The emission lines are shown to originate in H II regions. We estimated the metallicity from the intensity ratio of the [N II]λ6583 and Hα lines to be nearly solar, which rules out the possibility that the polar ring was produced by the accretion of gas from a dwarf companion.  相似文献   

On the mathematical description of fine structure under the conditions of weak variability     

G. A. Moiseev 《Physical Oceanography》1993,4(3):183-192

The idea of the weak variability of the fields is introduced, which means that when they are recorded by some measuring instrument (MI), the output signal obtains increments of the order of one/several quanta of sensitivity at the discreteness interval. At small scales (microstructure), this field is described in terms of random discrete values which reflect the properties of both the field measured and the MI. Theoretical relationships which define the probabilities of increments at the compound intervals in terms of the probabilities of increments at the sampling intervals, are derived for the case of independent random increments at the sampling intervals of discreteness. The validity of this model is illustrated by respective computations using data of microstructure measurements of the temperature profile in the main thermocline in the Sargasso Sea.Translated by Mikhail M. Trufanov.  相似文献   

Application of the global modal approach to the spiral galaxies     

Natalia Orlova  Vladimir Korchagin  Nobuhiro Kikuchi  Shoken. M. Miyama  Aleksei Moiseev 《Astrophysics and Space Science》2003,284(2):739-742

We have tested the applicability of the global modal approach in the density wave theory of spiral structure for a sample of spiral galaxies with measured axisymmetric background properties. We report here the results of the simulations for four galaxies: NGC 488, NGC 628, NGC 1566, and NGC 3938. Using the observed radial distributions for the stellar velocity dispersions and the rotation velocities we have constructed the equilibrium models for the galactic disks in each galaxy and implemented two kinds of stability analyses - the linear global analysis and 2D-nonlinear simulations. In general, the global modal approach is able to reproduce the observed properties of the spiral arms in the galactic disks. The growth of spirals in the galactic disks can be physically understood in terms of amplification by over-reflection at the corotation resonance. Our results support the global modal approach as a theoretical explanation of spiral structure in galaxies. This revised version was published online in August 2006 with corrections to the Cover Date.  相似文献   

Early-type disk galaxies: Structure and kinematics     

A. V. Zasov  A. V. Moiseev  A. V. Khoperskov  E. A. Sidorova 《Astronomy Reports》2008,52(2):79-93

Spectroscopic observations of three lenticular (S0) galaxies (NGC 1167, NGC 4150, and NGC 6340) and one SBa galaxy (NGC 2273) have been taken with the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences aimed to study the structure and kinematic properties of early-type disk galaxies. The radial profiles of the stellar radial velocities and the velocity dispersion are measured. N-body simulations are used to construct dynamical models of galaxies containing a stellar disk, bulge, and halo. The masses of individual components are estimated formaximum-mass disk models. A comparison of models with estimated rotational velocities and the stellar velocity dispersion suggests that the stellar disks in lenticular galaxies are “overheated”; i.e., there is a significant excess velocity dispersion over the minimum level required to maintain the stability of the disk. This supports the hypothesis that the stellar disks of S0 galaxies were subject to strong gravitational perturbations. The relative thickness of the stellar disks in the S0 galaxies considered substantially exceed the typical disk thickness of spiral galaxies.  相似文献   

Halo white dwarfs and the evolution of the galaxy     

D. S. Wiebe  A. V. Moiseev  Ya. A. Tikhonov  A. V. Tutukov  B. M. Shustov 《Astronomy Reports》2006,50(1):23-30

  相似文献   

Radio and optical spectra of objects from three complete samples of radio sources     

V. L. Afanas’ev  S. N. Dodonov  A. V. Moiseev  A. G. Gorshkov  V. K. Konnikova  M. G. Mingaliev 《Astronomy Reports》2006,50(4):255-272

We present classifications, optical identifications, and radio spectra for 19 radio sources from three complete samples, with declinations 4°–6° (B1950, S _{3.9 GHz} > 200 mJy), 10°–12°30′ (J2000, S _{4.85 GHz} > 200 mJy), and 74°–75° (J2000, S _{4.85 GHz} > 100 mJy). We also present corresponding information for the radio source J0527+0331. The right ascensions are 0–24^h and the Galactic latitudes |b| > 15° for all the samples. Our observations were obtained with the 6 m telescope from the Special Astrophysical Observatory in the range 4000–9000 Å or 4000–7500 Å and the RATAN-600 radio telescope at frequencies in the range 0.97–21.7 GHz. We obtained flux densities for the radio sources and optical spectra for their optical counterparts. Nine objects were classified as quasars with redshifts from z = 1.029 to 3.212; nine objects are emission-line galaxies with redshifts from 0.172 to 0.546, and one is a galaxy with burstlike star formation at z = 0.156, and one is a BL Lac object with z = 0.509. The spectra of five radio sources were decomposed into extended and compact components. The radio source J0527+0331, identified with a BL Lac object, displays significant variations of time scales from several days to several years. Data on flux variations are presented for 11 radio sources, as well as their spectra at several epochs.  相似文献   

Tectonic Position of the South Anyui Suture     

Sokolov  S. D.  Tuchkova  M. I.  Ledneva  G. V.  Luchitskaya  M. V.  Ganelin  A. V.  Vatrushkina  E. V.  Moiseev  A. V. 《Geotectonics》2021,55(5):697-716

Geotectonics - The South Anyui Fold System was formed at the end of the Early Cretaceous at the site of a closed oceanic basin as a result of the collision of the Chukotka microcontinent with the...  相似文献   

Volcanic-sedimentary complex of Otrozhnaya sheet in the Ust-Belaya Terrane,western Koryakia     

A. V. Moiseev  S. D. Sokolov  Ya. Hayasaka 《Geotectonics》2014,48(3):188-206

New data on the structure and composition of the rock complexes making up the Otrozhnaya sheet of the Ust-Belaya Terrane are discussed. This sheet is currently regarded as a complete section of the Early Devonian oceanic crust. The U-Pb age of zircon (547 ± 17 Ma) from plagiogranite porphyry that cuts through the ultramafic-gabbroic complex indicates that the country rocks are much older. Basalts of volcanic complex are similar to MORB-type rocks. The contact between volcanic and volcano-sedimentary complexes is tectonic. No volcanic-cherty association of rocks typical of ophiolites has been established at the base of the sedimentary sequence. The U-Pb age of detrital zircons from the base of this section is 571 Ma. As follows from the composition of terrigenous rocks and the suprasubduction origin of andesitic lavas and tuffs, the rocks of the lower part of volcano-sedimentary complex were deposited at the marginal part of the basin near convergent boundary. The remains of conodont elements make it possible to estimate the age of the upper part of the volcano-sedimentary complex as Late Devonian. The composition of terrigenous rocks shows that the provenance has abruptly changed. Sporadic rock fragments evidence the erosion of ophiolitic sections. Silurian rocks became the main source of clastic material. This is corroborated by redeposited microfauna species and U-Pb age of detrital zircons (～432 Ma). The geochemistry of dacite pebbles from conglomerate indicates that this volcanic rock was formed in a suprasuduction setting. The Ordovician-Silurian island arc could have been a source.  相似文献   

Reduction of CCD observations made with a scanning Fabry–Perot interferometer. III. Wavelength scale refinement     

A. V. Moiseev 《Astrophysical Bulletin》2015,70(4):494-500

  相似文献   

Galactic wind in NGC 4460: New observations     

D. V. Oparin  A. V. Moiseev 《Astrophysical Bulletin》2015,70(4):392-399

  相似文献