排序方式： 共有67条查询结果，搜索用时 31 毫秒
31.
A. E. Vol’vach L. N. Vol’vach A. M. Kut’kin M. G. Larionov M. Villata K. M. Panteri A. Lahteenmaki M. Tornikoski P. Savolainen G. Tammi A. F. Aller H. D. Aller S. G. Sergeev V. T. Doroshenko Yu. S. Efimov S. A. Klimanov S. V. Nazarov G. V. Borman A. B. Pushkarev V. I. Zhdanov E. V. Fedorova I. B. Vavilova N. G. Chesnok 《Astronomy Reports》2011,55(7):608-615
Long-term monitoring data at five radio frequencies from 4.8 to 37 GHz obtained at the Crimean Astrophysical Observatory, Metsahovi Radio Observatory of Aalto University, and the University of Michigan Radio Astronomy Observatory are used to analyze variations of the flux of the Active Galactic Nucleus (AGN) 3C 454.3. The dynamical characteristics of the three latest powerful flares from 2004 to 2010 are analyzed in detail. Observations in the gamma-ray (0.1–300 GeV), X-ray (2–10 kev, 15–50 keV), and optical are also used. Delays in the development of flares at different frequencies are derived. An empirical frequency dependence for the delays of flares from the gamma-ray to the radio is determined, which can be fit using a logarithmic low and remains the same from flare to flare. The physical characteristics of the central region of the AGN 3C 454.3 are used to estimate the size of its Strömgren sphere, taking into account the relevant mechanisms for heating and cooling the medium, as well as the adopted laws for the variation of the density and temperature with distance from the source of ionization. A model for the location of the radiation regions in the jet at various frequency ranges during the development of flares is proposed. 相似文献
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Vasilii V. Gvaramadze Alessia Gualandris Simon Portegies Zwart 《Monthly notices of the Royal Astronomical Society》2008,385(2):929-938
Recent proper motion and parallax measurements for the pulsar PSR B1508+55 indicate a transverse velocity of ∼1100 km s−1 , which exceeds earlier measurements for any neutron star. The spin-down characteristics of PSR B1508+55 are typical for a non-recycled pulsar, which implies that the velocity of the pulsar cannot have originated from the second supernova disruption of a massive binary system. The high velocity of PSR B1508+55 can be accounted for by assuming that it received a kick at birth or that the neutron star was accelerated after its formation in the supernova explosion. We propose an explanation for the origin of hyperfast neutron stars based on the hypothesis that they could be the remnants of a symmetric supernova explosion of a high-velocity massive star which attained its peculiar velocity (similar to that of the pulsar) in the course of a strong dynamical three- or four-body encounter in the core of dense young star cluster. To check this hypothesis, we investigated three dynamical processes involving close encounters between: (i) two hard massive binaries, (ii) a hard binary and an intermediate-mass black hole (IMBH) and (iii) a single stars and a hard binary IMBH. We find that main-sequence O-type stars cannot be ejected from young massive star clusters with peculiar velocities high enough to explain the origin of hyperfast neutron stars, but lower mass main-sequence stars or the stripped helium cores of massive stars could be accelerated to hypervelocities. Our explanation for the origin of hyperfast pulsars requires a very dense stellar environment of the order of 106 – 107 stars pc−3 . Although such high densities may exist during the core collapse of young massive star clusters, we caution that they have never been observed. 相似文献
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Alexey Vladimirovich Kargin Lyudmila Vyacheslavovna Sazonova Anna Andreevna Nosova Vladimir Anatolievich Pervov Elena Vladimirovna Minevrina Vladimir Anatolievich Khvostikov Zhanna Petrovna Burmii 《地学前缘(英文版)》2017,8(4):653-669
The petrography and mineral composition of a mantle-derived garnet peridotite xenolith from the V. Grib kimberlite pipe (Arkhangelsk Diamond Province, Russia) was studied. Based on petrographic characteristics, the peridotite xenolith reflects a sheared peridotite. The sheared peridotite experienced a complex evolution with formation of three main mineral assemblages: (1) a relict harzburgite assemblage consist of olivine and orthopyroxene porphyroclasts and cores of garnet grains (Gar1) with sinusoidal rare earth elements (REE) chondrite C1 normalized patterns; (2) a neoblastic olivine and orthopyroxene assemblage; (3) the last assemblage associated with the formation of clinopyroxene and garnet marginal zones (Gar2). Major and trace element compositions of olivine, orthopyroxene, clinopyroxene and garnet indicate that both the neoblast and clinopyroxene-Gar2 mineral assemblages were in equilibrium with a high Fe-Ti carbonate-silicate metasomatic agent. The nature of the metasomatic agent was estimated based on high field strength elements (HFSE) composition of olivine neoblasts, the garnet-clinopyroxene equilibrium condition and calculated by REE-composition of Gar2 and clinopyroxene. All these evidences indicate that the agent was a high temperature carbonate-silicate melt that is geochemically linked to the formation of the protokimberlite melt. 相似文献
35.
A. B. Pushkarev 《Astronomy Reports》2001,45(9):667-675
We present the results of multi-frequency polarization VLA observations of radio sources from the complete sample of northern, radio-bright BL Lac objects compiled by H. Kühr and G. Schmidt. These were used to determine the integrated rotation measures of 18 sources, 15 of which had never been measured previously, which hindered analysis of the intrinsic polarization properties of objects in the complete sample. These measurements make it possible to correct the observed orientations of the linear polarizations of these sources for the effect of Faraday rotation. The most probable origin for Faraday rotation in these objects is the Galactic interstellar medium. The results presented complete measurements of the integrated rotation measures for all 34 sources in the complete sample of BL Lac objects. 相似文献
36.
P. Yu. Pushkarev T. Ernst J. Jankowski W. Jozwiak M. Lewandowski K. Nowozynski V. Yu. Semenov 《Geophysical Journal International》2007,169(3):926-940
The deep resistivity structure was estimated along a 400-km profile in central Poland crossing the Malopolska Massif (MM), the Lysogory Unit (LU), the Trans-European Suture Zone (TESZ) and ending at the East European Craton (EEC). Magnetotelluric transfer functions, corresponding to 20 sites, were supplemented by magnetovariational responses obtained at the geomagnetic observatories situated at the same tectonic units. Such a combination made it possible to extend the initial period range, which is from fractions of a second to several hours, up to months in order to reliably cover crustal and upper-mantle depths. The geoelectrical structures, revealed using 2-D inversions, do not contradict the known features of the lithosphere structure determined using seismic and gravity data along the profile.
The subsurface conductance, varying from approximately 10 Siemens at the inner part of the EEC to about 600 Siemens in the TESZ, is produced by sediments, the deep part of which contains conductive, highly mineralized water. The existence of two crustal conductive faults at the southwest and northeast of the TESZ were established mainly by the use of induction arrows. It was also revealed that rather high mantle conductivity beneath the MM, LU and TESZ at depths of about 150–200 km contrasts with the resistive upper mantle of the EEC. This can be interpreted as the decrease of asthenosphere conductance and/or as its submersion beneath the EEC. Generally, the results confirm the idea that the TESZ forms not only specific seismic boundaries but also causes peculiar conductivity anomalies in the crust and upper mantle. 相似文献
The subsurface conductance, varying from approximately 10 Siemens at the inner part of the EEC to about 600 Siemens in the TESZ, is produced by sediments, the deep part of which contains conductive, highly mineralized water. The existence of two crustal conductive faults at the southwest and northeast of the TESZ were established mainly by the use of induction arrows. It was also revealed that rather high mantle conductivity beneath the MM, LU and TESZ at depths of about 150–200 km contrasts with the resistive upper mantle of the EEC. This can be interpreted as the decrease of asthenosphere conductance and/or as its submersion beneath the EEC. Generally, the results confirm the idea that the TESZ forms not only specific seismic boundaries but also causes peculiar conductivity anomalies in the crust and upper mantle. 相似文献
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Valeriy P. Bubnov Andrey G. Yakovlev Elena D. Aleksanova Denis V. Yakovlev Mark N. Berdichevsky Pavel Yu. Pushkarev 《Acta Geophysica》2007,55(2):154-168
Magnetotelluric method is widely applied to study the Russian part of the East-European Craton, as well as the Caucasus and
the Urals: several thousand soundings were performed during the last few years. Their periods range is approximately from
0.003 to 3000 seconds, which allows to study the sedimentary cover and the consolidated crust. Resistivity cross-sections
along several regional profiles which run across the tectonic structures of the East-European Craton and the adjacent folded
systems were obtained, mainly using 1D and 2D interpretational tools. MT investigations provided important information about
the structure and reservoir properties of sedimentary complexes, the state of active geodynamic regions, the graphitization
and fluid regime of the consolidated crust, and the permeable and fluid-saturated crustal zones. 相似文献
39.
Astronomy Reports - Different astrophysical objects, such as the Sun, another stars, galaxies and accretion discs have regular magnetic field structures. Their generation is usually connected with... 相似文献
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Ivanov P. V. Varentsov Iv. M. Kolodyazhnyi S. Yu. Lozovsky I. N. Pushkarev P. Yu. Rodina T. A. 《Izvestiya Physics of the Solid Earth》2022,58(5):626-641
Izvestiya, Physics of the Solid Earth - Abstract—The geoelectric structure of the junction region between three largest segments of the East European Craton (EEC)–Volga–Uralia,... 相似文献