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19912026
most citedPlanck 2015 results. XIII. Cosmological parameters

10.6k citations

Showing 2004 · astro-phShow all

30 papers · 2 filters

astro-ph2004★ 14 cited

Two-dimensional structure of thin transonic discs: theory and observational manifestations

V. S. Beskin, A. D. Tchekhovskoy

We study the two-dimensional structure of thin transonic accretion discs in the vicinity of black holes. We use the hydrodynamical version of the Grad-Shafranov equation and focus…

astro-ph2004★ 2 cited

The iron -line as a tool for an evaluation of black hole parameters

A. F. Zakharov

Recent X-ray observations of microquasars and Seyfert galaxies reveal broad emission lines in their spectra, which can arise in the innermost parts of accretion disks. Simulations…

astro-ph2004★ 71 cited

Optical and GeV-TeV flashes from gamma-ray bursts

Andrei M. Beloborodov

The synchrotron optical flash caught in GRB 990123 overlaps with the MeV radiation front, and the optical-emitting electrons must also produce GeV-TeV emission by inverse Compton s…

astro-ph2004★ 117 cited

Mirages around Kerr black holes and retro-gravitational lenses

A. F. Zakharov, A. A. Nucita, F. DePaolis +1

Recently Holz & Wheeler (2002) considered a very attracting possibility to detect retro-MACHOs, i.e. retro-images of the Sun by a Schwarzschild black hole. In this paper we discuss…

astro-ph2004

Polarization and energy content of parsec scale AGN jets

Maxim Lyutikov, Vladimir I. Pariev, Denise C. Gabuzda

Most of energy carried by relativistic AGN jets remains undetected until hundreds of kiloparsecs where interaction with intergalactic medium produces hot spots. The jet's hidden en…

astro-ph2004★ 4 cited

Models and phenomenology

A. D. Erlykin

It is evident that models of the knee should match the observational phenomenology. In this talk I discuss a few aspects of phenomenology, which are important not only for the unde…

astro-ph2004★ 17 cited

Hard X-ray Emission Clumps in the gamma-Cygni Supernova Remnant: an INTEGRAL-ISGRI View

A. M. Bykov, A. M. Krassilchtchikov, Yu. A. Uvarov +12

Spatially resolved images of the galactic supernova remnant G78.2+2.1 (gamma-Cygni) in hard X-ray energy bands from 25 keV to 120 keV are obtained with the IBIS-ISGRI imager aboard…

astro-ph2004★ 7 cited

The Maximum Energy and Spectra of Cosmic Rays Accelerated in Active Galactic Nuclei

A. V. Uryson

We computed the energy spectra of the incident (on an air shower array) ultrahigh-energy (E > 4x10^19 eV) cosmic rays (CRs) that were accelerated in nearby Seyfert nuclei at redshi…

astro-ph2004★ 162 cited

The Third VLBA Calibrator Survey

L. Petrov, Y. Y. Kovalev, E. Fomalont +1

This paper presents the third extension to the Very Large Baseline Array (VLBA) Calibrator Survey, containing 360 new sources not previously observed with very long baseline interf…

astro-ph2004★ 1 cited

Contribution of microlensing to X-ray variability of distant QSOs

Alexander F. Zakharov, Luka C. Popovic, Predrag Jovanovic

We consider a contribution of microlensing to the X-ray variability of high-redshifted QSOs. Cosmologically distributed gravitational microlenses could be localized in galaxies (or…

astro-ph2004★ 16 cited

The Interplanetary Network Supplement to the BATSE Catalogs of Untriggered Cosmic Gamma Ray Bursts

K. Hurley, B. Stern, J. Kommers +16

We present Interplanetary Network (IPN) detection and localization information for 211 gamma-ray bursts (GRBs) observed as untriggered events by the Burst and Transient Source Expe…

astro-ph2004★ 28 cited

Accretion disks around Black Holes with Advection and Optical Depth Transition

Yu. V. Artemova, G. S. Bisnovatyi-Kogan, I. V. Igumenshchev +1

We consider the effects of advection and radial gradients of pressure and radial drift velocity on the structure of accretion disks around black holes with proper description of op…

astro-ph2004★ 2 cited

A new method for the UHECR mass composition studies

M. Ambrosio, C. Aramo, D. D'Urso +3

The detemination of the primary cosmic ray mass composition from the longitudinal development of atmospheric cascades is still an open problem. In this work we propose a new method…

astro-ph2004★ 153 cited

The tidal disruption rate in dense galactic cusps containing a supermassive binary black hole

P. B. Ivanov, A. G. Polnarev, P. Saha

We consider the problem of tidal disruption of stars in the centre of a galaxy containing a supermassive binary black hole with unequal masses. We assume that over the separation d…

astro-ph2004★ 9 cited

On the structure of line-driven winds near black holes

A. V. Dorodnitsyn, I. D. Novikov

A general physical mechanism of the formation of line-driven winds at the vicinity of strong gravitational field sources is investigated in the frame of General Relativity. We argu…

astro-ph2004★ 120 cited

Giant Pulses from PSR B1937+21 with widths <= 15 nanoseconds and T_b >= 5 x 10^39 K, the Highest Brightness Temperature Observed in the Universe

V. A. Soglasnov, M. V. Popov, N. Bartel +4

Giant radio pulses of the millisecond pulsar B1937+21 were recorded with the S2 VLBI system at 1.65 GHz with NASA/JPL's 70-m radio telescope at Tidbinbilla, Australia. These pulses…

astro-ph2004★ 128 cited

High Energy Emission from Magnetars

C. Thompson, A. M. Beloborodov

The recently discovered soft gamma-ray emission from the anomalous X-ray pulsar 1E 1841-045 has a luminosity L_g ~ 10^{36} ergs/s. This luminosity exceeds the spindown power by thr…

astro-ph2004★ 2 cited

'Sling effect' in the development of atmospheric cascades induced by primary cosmic ray nuclei

A. D. Erlykin, A. W. Wolfendale

The 'Sling effect' appears when a fragment of a projectile nucleus emitted after its peripheral collision with a target nucleus is caused to rotate with a high spin. The spinning f…

astro-ph2004★ 83 cited

Gamma-ray bursts from synchrotron self-Compton emission

Boris E. Stern, Juri Poutanen

The emission mechanism of the gamma-ray bursts (GRBs) is still a matter of debates. The standard synchrotron energy spectrum of cooling electrons F_E ~ E^{-1/2} is much too soft to…

astro-ph2004★ 11 cited

PSR B0809+74: Understanding Its Perplexing Subpulse-separation (P2) Variations

Joanna M. Rankin, R. Ramachandran, Svetlana A. Suleymanova

The longitude separation between adjacent drifting subpulses, , is roughly constant for many pulsars. It was then perplexing when pulsar B0809+74 was found to exhibit substant…

astro-ph2004★ 258 cited

Polarization and structure of relativistic parsec-scale AGN jets

Maxim Lyutikov, Vladimir I. Pariev, Denise C. Gabuzda

(Abridged) We consider the polarization properties of optically thin synchrotron radiation emitted by relativistically moving electron--positron jets carrying large-scale helical m…

astro-ph2004★ 23 cited

Orbital roulette: a new method of gravity estimation from observed motions

Andrei M. Beloborodov, Yuri levin

The traditional way of estimating the gravitational field from observed motions of test objects is based on the virial relation between their kinetic and potential energy. We find…

astro-ph2004★ 18 cited

Foreground analysis from the 1-year Wilkinson Microwave Anisotropy Probe (WMAP) data

Pavel D. Naselsky, Oleg V. Verkhodanov, Lung-Yih Chiang +1

We present a detailed analysis on the phases of the WMAP foregrounds (synchrotron, free-free and dust emission) of the WMAP K-W bands in order to estimate the significance of the v…

astro-ph2004★ 32 cited

Cosmic Rays and the Monogem Supernova Remnant

A. D. Erlykin, A. W. Wolfendale

Recent findings indicate that the Monogem Ring supernova remnant (SNR) and the associated pulsar B0656+14 may be the 'Single Source' responsible for the knee in the cosmic ray (CR)…