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20002026
most citedThe Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission

395 citations · 5.4k across the 130 of their papers we have counts for

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Showing 2009Show all

7 papers · 1 filter

astro-ph.CO2009★ 28 cited

Remarkable Spectral Variability of PDS 456

Ehud Behar, Shai Kaspi, James Reeves +3

We report on the highest to date signal-to-noise-ratio X-ray spectrum of the luminous quasar PDS 456, as obtained during two XMM-Newton orbits in September 2007. The present spectr…

astro-ph.GA2009★ 27 cited

X-Ray Absorption Analysis of MCG-6-30-15: Discerning Three Kinematic Systems

Tomer Holczer, Ehud Behar, Nahum Arav

By analyzing the X-ray spectrum of MCG-6-30-15 obtained with the HETG spectrometer on board the Chandra Observatory, we identify three kinematically distinct absorption systems; tw…

astro-ph.HE2009★ 191 cited

MHD Accretion-Disk Winds as X-ray Absorbers in AGNs

Keigo Fukumura, Demosthenes Kazanas, Ioannis Contopoulos +1

We present the 2D ionization structure of self-similar MHD winds off accretion disks around irradiated by a central X-ray source. Based on earlier observational clues and theoretic…

astro-ph.SR2009★ 11 cited

XMM-Newton detection of a transient X-ray source in the vicinity of V838 Monocerotis

Fabio Antonini, Rodolfo Jr. Montez, Joel H. Kastner +5

We report the XMM-Newton/EPIC detection in 2008 March of a luminous (L_X ~ 10^32-33 erg/s), variable X-ray source in the vicinity (within ~6") of the enigmatic star V838 Mon, which…

astro-ph.GA2009★ 90 cited

Density Profiles in Seyfert Outflows

Ehud Behar

For the past decade, ionized outflows of a few 100 km/s from nearby Seyfert galaxies have been studied in great detail using high resolution X-ray absorption spectra. A recurring f…

astro-ph.HE2009★ 197 cited

A Compton-thick Wind in the High Luminosity Quasar, PDS 456

J. N. Reeves, P. T. O'Brien, V. Braito +7

PDS 456 is a nearby (z=0.184), luminous (L_bol ~10^47 erg/s) type I quasar. A deep 190 ks Suzaku observation in February 2007 revealed the complex, broad band X-ray spectrum of PDS…

astro-ph.HE2009★ 15 cited

Narrow Radiative Recombination Continua: A Signature of Ions Crossing the Contact Discontinuity of Astrophysical Shocks

Raanan Nordon, Ehud Behar, Noam Soker +2

X-rays from planetary nebulae (PNs) are believed to originate from a shock driven into the fast stellar wind (v ~ 1000 km/s) as it collides with an earlier circumstellar slow wind…