New outcrop of buried Kazantsevo peat at lower reaches of the Irtysh River     

S. A. Laukhin  Kh. A. Arslanov  F. E. Maksimov  V. Yu. Kuznetsov  G. N. Shilova  F. Yu. Velichkevich  S. B. Chernov  Ya. A. Nikonorov 《Doklady Earth Sciences》2008,419(2):200-204

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Geochronology and landscape-climatic environments of the Early Zyryanian Interstadial in West Siberia     

S. A. Laukhin  F. E. Maksimov  Kh. A. Arslanov  V. Yu. Kuznetsov  S. B. Chernov  G. N. Shilova  F. Yu. Velichkevich 《Doklady Earth Sciences》2008,421(1):796-799

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Structure features of convective channels from thermal sources in Mutnovskii volcano (South Kamchatka)     

Yu. A. Manshtein  S. B. Bortnikova  A. K. Manshtein  G. M. Gavrilenko  I. V. Vernikovskaya  N. P. Sez’ko 《Doklady Earth Sciences》2008,423(2):1404-1409

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Cretaceous-Paleogene back-arc basins in the Iran-Afghanistan-Pamirs segment of the Eurasian active margin     

V. G. Kaz’min  N. F. Tikhonova 《Doklady Earth Sciences》2008,422(1):1018-1020

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Late Quaternary marine terraces in the Mediterranean coastal area of Syria: Geochronology and neotectonics     

A.E. Dodonov  V.G. Trifonov  T.P. Ivanova  V.Yu. Kuznetsov  F.E. Maksimov  D.M. Bachmanov  T.A. Sadchikova  A.N. Simakova  H. Minini  A.-M. Al-Kafri  O. Ali 《Quaternary International》2008,190(1):158

In order to provide new data on the neotectonics and geodynamic properties of western Syria, studies of marine terraces have been carried out. The most attention was paid to the lower terraces in the range of 3–5 to 30–35 m above sea level, because they have more complete distributions along the shore. The lower terraces were examined along the coastal area from Tartus to Latakia, and along the carbonate cliff on Arwad Island. Seven ²³⁰Th/U dates for these terraces are in the range of 85–130 ka, suggesting the age interval of the last interglacial (MIS 5). New dates on the lower terraces provide a basis for stratigraphical and geomorphological interpretation as well as neotectonic reconstruction. According to the geomorphological data and lithological composition of those terraces, two main uplifted blocks can be established. One coincides with the Latakia block, and another corresponds to the western margin of the Banias volcanic plateau. These blocks are divided by a subsided structure corresponding to the Nahr el Kebir graben. The amplitude of neotectonic uplifting in the Latakia and Banias blocks reaches 15–20 m for the Late Pleistocene.  相似文献   

The structure of the tectonosphere of the Urals and West Siberian Platform by electromagnetic data     

A. G. D’yakonova  K. S. Ivanov  O. V. Surina  P. F. Astaf’ev  V. S. Vishnev  A. D. Konoplin 《Doklady Earth Sciences》2008,423(2):1479-1482

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Climatic changes and alluvial-sedimentation settings in southeastern Transbaikalia in the Middle-Late Holocene (by the example of the Ilya floodplain)     

V.B. Bazarova  L.M. Mokhova  M.A. Klimin  L.A. Orlova  K.Yu. Bazarov 《Russian Geology and Geophysics》2008,49(12):978-985

Climatic changes in southeastern Transbaikalia in the Middle and Late Holocene and their influence on alluvial sedimentation environments are reconstructed from the results of study of the Ilya floodplain sediments (Alkhanai National Park). At the beginning of the Subboreal period, the regional climate became more arid, which led to a significant increase in steppe species communities in the landscapes. Intense climate aridization also took place at the beginning and at the end of the Subatlantic period of the Holocene. The alluvial-sedimentation rate increased during the weakening of aridization and decreased during cooling and the intensification of aridization. The obtained regional data are compared with data on the adjacent areas and the global climatic changes in the Northern Hemisphere.  相似文献   

Long-term variability of a complete sample of flat-spectrum radio sources at declinations of 4°–6° (B1950)     

A. G. Gorshkov  V. K. Konnikova  M. G. Mingaliev 《Astronomy Reports》2008,52(4):278-298

We present the results of twenty-year observations of a complete sample of 68 flat-spectrum radio sources with flux densities S _{3.9 GHz} > 200 mJy carried out at centimeter wavelengths with the RATAN-600 radio telescope. Since 1995, we have observed simultaneously at six frequencies between 0.97 and 21.7 GHz. Of the 56 sources identified with optical objects, 41 are quasars with redshifts between 0.293 and 3.263. Based on our analysis of the spectral shapes, we divide the sources into four classes. Changes of spectral class for individual sources are fairly rare. Based on the light curves and spectra, in most cases, a flare’s evolution is in accordance with a model in which the variations result from the evolution of a shock in the radio jet. The main result of our study is that there is no redshift dependence for the true linear sizes of the radiating regions, the variability indices derived for all 20 years of data or for individual flares, or the peak frequencies of the spectra of the compact radio emission. We suggest that this testifies to an absence of cosmological evolution of the sample quasars, at least to z ≈ 3.  相似文献   

The mass of the compact object in the X-ray binary her X-1/HZ her     

M. K. Abubekerov  E. A. Antokhina  A. M. Cherepashchuk  V. V. Shimanskii 《Astronomy Reports》2008,52(5):379-389

We have obtained the first estimates of the masses of the components of the Her X-1/HZ Her X-ray binary system taking into account non-LTE effects in the formation of the H _γ absorption line: m _x = 1.8 M _⊙ and m _v = 2.5 M _⊙. These mass estimates were made in a Roche model based on the observed radial-velocity curve of the optical star, HZ Her. The masses for the X-ray pulsar and optical star obtained for an LTE model lie are m _x = 0.85 ± 0.15 M _⊙ and m _v = 1.87 ± 0.13 M _⊙. These mass estimates for the components of Her X-1/HZ Her derived from the radial-velocity curve should be considered tentative. Further mass estimates from high-precision observations of the orbital variability of the absorption profiles in a non-LTE model for the atmosphere of the optical component should be made.  相似文献   

Spectroscopic monitoring of SS 433: A search for long-term variations of kinematic model parameters     

V. V. Davydov  V. F. Esipov  A. M. Cherepashchuk 《Astronomy Reports》2008,52(6):487-506

Between 1994 and 2006, we obtained uniform spectroscopic observations of SS 433 in the region of Hα. We determined Doppler shifts of the moving emission lines, Hα ₊ and Hα _?, and studied various irregularities in the profiles for the moving emission lines. The total number of Doppler shifts measured in these 13 years is 488 for Hα _? and 389 for Hα ₊. We have also used published data to study possible long-term variations of the SS 433 system, based on 755 Doppler shifts for Hα _? and 630 for Hα ₊ obtained over 28 years. We have derived improved kinematic model parameters for the precessing relativistic jets of S S 433 using five-and eight-parameter models. On average, the precession period was stable during the 28 years of observations (60 precession cycles), at 162.250^d ± 0.003^d. Phase jumps of the precession period and random variations of its length with amplitudes of ≈6% and ≈1%, respectively, were observed, but no secular changes in the precession period were detected. The nutation period, P _nut = 6.2876^d ± 0.00035^d, and its phase were stable during 28 years (more than 1600 nutation cycles). We find no secular variations of the nutation cycle. The ejection speed of the relativistic jets, v, was, on average, constant during the 28 years, β = v/c = 0.2561 ± 0.0157. No secular variation of β is detected. In general, S S 433 demonstrates remarkably stable long-term characteristics of its precession and nutation, as well as of the central “engine” near the relativistic object that collimates the plasma in the jets and accelerates it to v = 0.2561c. Our results support a model with a “slaved” accretion disk in S S 433, which follows the precession of the optical star’s rotation axis.  相似文献