activity
20012011
most citedOn the origin of radio emission in radio quiet quasars

228 citations · 530 across the 13 of their papers we have counts for

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Showing 2005Show all

8 papers · 1 filter

astro-ph2005

Inner-shell Absorption Lines of Fe~VI-- Fe~XVI: A Many-body Perturbation Theory Approach

Ming F. Gu, Tomer Holczer, Ehud Behar +1

We provide improved atomic calculation of wavelengths, oscillator strengths, and autoionization rates relevant to the inner-shell transitions of Fe~VI--XVI, the so-called…

astro-ph2005

The High-Velocity Outflow of PG 1211+143: An Unbiased View Based on Several Observations

Shai Kaspi, Ehud Behar

We present and discuss high-resolution grating spectra of the quasar PG1211+143 obtained over three years. Based on an early observation from 2001, we find an outflow component of…

astro-ph2005

Principal component analysis of the X-ray variability in NGC 7469

A. J. Blustin, S. V. Fuerst, G. Branduardi-Raymont +3

We apply Principal Component Analysis (PCA) to study the variability of the X-ray continuum in the Seyfert 1 galaxy NGC 7469. The PCA technique is used to separate out linear compo…

astro-ph2005

The High-Velocity Outflow of PG1211+143 May Not be That Fast

Shai Kaspi, Ehud Behar

We analyze the X-ray spectrum of the quasar PG1211+143 observed with the CCD and grating spectrometers on board XMM-Newton. Using an ion by ion fitting model we find an outflow com…

astro-ph2005

Accretion onto the Companion of Eta Carinae During the Spectroscopic Event: II. X-Ray Emission Cycle

Muhammad Akashi, Noam Soker, Ehud Behar

We calculate the X-ray luminosity and light curve for the stellar binary system Eta Carinae for the entire orbital period of 5.54 years. By using a new approach we find, as suggest…

astro-ph2005

X-Ray Emission by A Shocked Fast Wind from the Central Stars of Planetary Nebulae

Muhammad Akashi, Noam Soker, Ehud Behar

We calculate the X-ray emission from the shocked fast wind blown by the central stars of planetary nebulae (PNs) and compare with observations. Using spherically symmetric self sim…