3,156 research outputs found
Interpreting radiative efficiency in radio-loud AGNs
Author submitted version of unrefereed Nature Astronomy comment. Version in journal format available at https://rdcu.be/KH6WRadiative efficiency in radio-loud active galactic nuclei is governed by the accretion rate onto the central black hole rather than directly by the type of accreted matter; while it correlates with real differences in host galaxies and environments, it does not provide unambiguous information about particular objects.Non peer reviewedFinal Accepted Versio
Gravitational potential of a homogeneous circular torus: new approach
The integral expression for gravitational potential of a homogeneous circular
torus composed of infinitely thin rings is obtained. Approximate expressions
for torus potential in the outer and inner regions are found. In the outer
region a torus potential is shown to be approximately equal to that of an
infinitely thin ring of the same mass; it is valid up to the surface of the
torus. It is shown in a first approximation, that the inner potential of the
torus (inside a torus body) is a quadratic function of coordinates. The method
of sewing together the inner and outer potentials is proposed. This method
provided a continuous approximate solution for the potential and its
derivatives, working throughout the region.Comment: 10 pages, 9 figures, 1 table; some misprints in formulae were
correcte
The last Gift of BeppoSAX: PDS Observations of the two Blazars 1ES 0507-040 and PKS 1229-021
Towards the end of the BeppoSAX mission, the only operated Narrow Field
Instrument was the PDS, which covers the energy range 13-300 keV. Two blazars,
1ES 0507-040 (z=0.304) and PKS 1229-021 (z= 1.045), suitably located in the sky
for BeppoSAX pointing, were observed for about 2 days each in Spring 2002 with
the PDS and detected up to 50 keV. 1ES0507-040 had been already observed by the
BeppoSAX NFIs at an earlier epoch for a much shorter time. We have re-analysed
those data as well, and identified a possible contamination problem in the PDS
spectrum. We present our recent PDS data on both sources, combined with the
previous BeppoSAX data and with non-simultaneous observations at other
frequencies. The derived Spectral Energy Distributions allow us to discuss the
origin of the high energy component.Comment: 4 pages, 6 figures, poster presented at the symposium: The Restless
High-Energy Universe, Amsterdam, May 200
Swift XRT and UVOT deep observations of the high energy peaked BL Lac object PKS 0548-322 close to its brightest state
We present the results of a spectral analysis of 5 Swift XRT and UVOT
observations of the BL Lac object PKS 0548-322 carried out over the period
April-June 2005. The X-ray flux of this high energy peaked BL Lac (HBL) source
was found to be approximately constant at a level of F(2-10 keV) ~ 4x10^-11 erg
cm^-2 s^-1, a factor of 2 brighter than when observed by BeppoSAX in 1999 and
close to the maximum intensity reported in the Einstein Slew Survey. The very
good statistics obtained in the 0.3-10 keV Swift X-ray spectrum allowed us to
detect highly significant deviations from a simple power law spectral
distribution. A log-parabolic model describes well the X-ray data and gives a
best fit curvature parameter of 0.18 and peak energy in the Spectral Energy
Distribution of about 2 keV. The UV spectral data from Swift UVOT join well
with a power law extrapolation of the soft X-ray data points suggesting that
the same component is responsible for the observed emission in the two bands.
The combination of synchrotron peak in the X-ray band and high intensity state
confirms PKS 0548-322 as a prime target for TeV observations. X-ray monitoring
and coordinated TeV campaigns are highly advisable.Comment: Accepted for publication in A&A (6 pages, 3 figures
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