activity
19972009
most citedDynamics and High Energy Emission of the Flaring HST-1 Knot in the M 87 Jet

166 citations · 748 across the 18 of their papers we have counts for

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astro-ph2003

X-Ray Emission from the Quasar PKS 1127-145: Comptonized IR Photons on Parsec Scales

Michal Blazejowski, Aneta Siemiginowska, Marek Sikora +2

We model the broad-band spectral energy distribution of the innermost "core-jet" region of the redshift z=1.187 quasar PKS 1127-145. We propose a scenario where the high energy pho…

astro-ph2003

On the turbulent -disks and the intermittent activity in AGN

Agnieszka Janiuk, Bozena Czerny, Aneta Siemiginowska +1

We consider effects of the MHD turbulence on the viscosity during the evolution of the thermal-viscous ionization instability in the standard -accretion disks. We consider the p…

astro-ph2003

An X-ray jet discovered by Chandra in the z=4.3 radio-selected quasar GB 1508+5714

Aneta Siemiginowska, Randall K. Smith, Thomas L. Aldcroft +3

We report the Chandra discovery of an X-ray jet associated with the redshift 4.3 radio-loud quasar GB 1508+5714. The jet X-ray emission peaks ~2 arcsec to the South-West of the qua…

astro-ph2003

The origin of emission and absorption features in Ton S180 Chandra observations

A. Różańska, B. Czerny, A. Siemiginowska +2

We present new interpretation of Ton S180 spectrum obtained by {\it Chandra} Spectrometer (Low Energy Transmission Grating). Several narrow absorption lines and a few emission disk…

astro-ph2003

Constraints on AGN accretion disc viscosity derived from continuum variability

Rhaana L. C. Starling, Aneta Siemiginowska, Phil Uttley +1

We estimate a value of the viscosity parameter in AGN accretion discs for the PG quasar sample. We assume that optical variability on time-scales of months to years is caused by lo…

astro-ph2003

Chandra Observation of 3C 212: a New Look at the X-ray and UV Absorbers

T. L. Aldcroft, A. Siemiginowska, M. Elvis +3

The red quasar 3C 212 (z=1.049) is one of the most distant and most luminous AGN which has shown evidence of an X-ray warm absorber. In order to further investigate this unusual qu…