Transcurrent nature of the Teisseyre–Tornquist Zone in Central Europe: results of the POLCRUST-01 deep reflection seismic profile     

M. Narkiewicz  A. Maksym  M. Malinowski  M. Grad  A. Guterch  Z. Petecki  J. Probulski  T. Janik  M. Majdański  P. Środa  W. Czuba  E. Gaczyński  L. Jankowski 《International Journal of Earth Sciences》2015,104(3):775-796

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RC J0311+0507: A candidate for superpowerful radio galaxies in the early universe at redshift z = 4.514     

A. I. Kopylov  W. M. Goss  Yu. N. Pariĭskiĭ  N. S. Soboleva  O. V. Verkhodanov  A. V. Temirova  O. P. Zhelenkova 《Astronomy Letters》2006,32(7):433-438

A strong emission line at 6703 Å has been detected in the optical spectrum for the host galaxy (R = 23.1) of the radio source RC J0311+0507 (4C+04.11). This radio galaxy, with a spectral index of 1.31 in the frequency range 365–4850 MHz, is one of the ultrasteep-spectrum objects from the deep survey of a sky strip conducted with RATAN-600 in 1980–1981. We present arguments in favor of the identification of this line with Lyα at redshift z = 4.514. In this case, the object belongs to the group of extremely distant radio galaxies of ultrahigh radio luminosity (P ₁₄₀₀ = 1.3 × 10²⁹ W Hz^?1). Such power can be provided only by a fairly massive black hole (～10⁹ M⊙) that formed in a time less than the age of the Universe at the observed z (1.3 Gyr) or had a primordial origin.  相似文献   

Regional dynamics of socio-economic change —The experiences and prospects in sparsely populated areas     

Antoni Kukliński Prof. Dr. 《GeoJournal》1986,12(1):107-110

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Black hole spin in GRS 1915+105   总被引：2，自引：0，他引：2  

Matthew Middleton  Chris Done  Marek Gierli&#;ski  Shane W. Davis 《Monthly notices of the Royal Astronomical Society》2006,373(3):1004-1012

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Statistical characteristics of the observed Lyα forest and the shape of the initial power spectrum     

M. Demia&#;ski  A. G. Doroshkevich  V. I. Turchaninov 《Monthly notices of the Royal Astronomical Society》2006,371(2):915-934

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Be star candidates in the Large Magellanic Cloud: the catalogue and comparison with the Small Magellanic Cloud sample     

B. E. Sabogal  R. E. Mennickent  G. Pietrzy&#;ski  W. Gieren 《Monthly notices of the Royal Astronomical Society》2005,361(3):1055-1062

We present a catalogue with coordinates and photometric data of 2446 Be star candidates in the Large Magellanic Cloud (LMC), based on a search of the OGLE II data base. The I -band light curves of these stars show outbursts in 24 per cent of the sample (Type-1 stars), high and low states in 10 per cent, periodic variations in 6 per cent (Type-3 stars), and stochastic variations in 60 per cent of the cases. We report on the result of the statistical study of light curves of Type-1 and Type-3 stars in the LMC, and the comparison with the previously reported results of the Small Magellanic Cloud (SMC) sample. We find a statistically significant difference between amplitude, duration and asymmetry distributions of outbursts in both galaxies. Outbursts of SMC Type-1 stars are usually brighter, longer and with a slower decline. We find a bimodal distribution of periods of Type-3 stars in both galaxies, probably related to the recently discovered double periodic blue variables. We find also period and amplitude distributions of Type-3 LMC stars statistically different from those of the SMC stars. Our findings above suggest that the mechanisms causing the observed photometric variability of Type-1 and Type-3 stars could depend on metallicity. Moreover, they suggest that the outbursts are not primarily caused by stellar winds.  相似文献   

GRS 1915+105: the brightest Galactic black hole     

Chris Done  Grzegorz Wardzi&#;ski  Marek Gierli&#;ski 《Monthly notices of the Royal Astronomical Society》2004,349(2):393-403

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Book reviews     

Roy  B. K.  Stanley  William R.  Bronger  Dirk  Dlin  Norman  Kukliński  Antoni  Cori  Berardo  Babikir  A. A. A.  Kunkel  G.  César  N.  Martin  Kähler 《GeoJournal》1989,18(2):255-260

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Discovery of powerful millisecond flares from Cygnus X-1     

Marek Gierli&#;ski  Andrzej A. Zdziarski 《Monthly notices of the Royal Astronomical Society》2003,343(3):L84-L88

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The asymmetry of the velocity distribution in the rotating ring in U Gem stars     

B. Paczyński  S. L. Piotrowski  W. Turski 《Astrophysics and Space Science》1968,2(2):254-257

It is shown that the non-keplerian character of the rotation of the ring of gas particles in a close binary system gives too large an amplitude of the radial velocity curve if this amplitude is determined from the positions of the emission lines of the ring.  相似文献