activity
19942008
most citedTheoretical current-voltage characteristics of ferroelectric tunnel junctions

435 citations · 1.3k across the 79 of their papers we have counts for

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astro-ph2008

Optical identification of a new cataclysmic variable from integral all sky survey: IGR J08390--4833

M. Revnivtsev, A. Kniazev, S. Sazonov +6

We have optically identified a recently discovered INTEGRAL source, IGR J08390--4833, with a cataclysmic variable, i.e. an accreting white dwarf in a binary system. The spectrum ex…

astro-ph200823 cited

Serendipitous VLBI detection of rapid, large-amplitude, intraday variability in QSO 1156+295

T. Savolainen, Y. Y. Kovalev

We report a serendipitous detection of rapid, large amplitude flux density variations in the highly core-dominated, flat-spectrum radio quasar 1156+295 during an observing session…

astro-ph2008

Stellar populations and galaxy evolution in the NGC 80 group

Olga K. Silchenko, Victor L. Afanasiev

We have studied the central parts of seven early-type galaxies -- the members of the X-ray-bright galaxy group NGC 80 -- by means of integral-field spectroscopy at the Russian 6m t…

astro-ph2008106 cited

An Extreme Solar Event of 20 January 2005: Properties of the Flare and the Origin of Energetic Particles

V. V. Grechnev, V. G. Kurt, I. M. Chertok +9

The extreme solar and SEP event of 20 January 2005 is analyzed from two perspectives. Firstly, we study features of the main phase of the flare, when the strongest emissions from m…

astro-ph200721 cited

Superorbital variability of X-ray and radio emission of Cyg X-1. I. Emission anisotropy of precessing sources

A. Ibragimov, A. A. Zdziarski, J. Poutanen

We study theoretical interpretations of the 150-d (superorbital) modulation observed in X-ray and radio emission of Cyg X-1 in the framework of models connecting this phenomenon to…

astro-ph20071 cited

A cool R Coronae Borealis star Z UMi

Tonu Kipper, Valentina Klochkova

The high resolution spectra of a R CrB type star Z UMi are analysed. The atmospheric parameters of Z UMi are estimated: Teff=5250+/-250K and log g=0.5+/-0.3. This places Z UMi amon…