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19942026
most citedThe Axisymmetric Pulsar Magnetosphere

480 citations · 6k across the 156 of their papers we have counts for

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55 papers · 1 filter

astro-ph2008★ 3 cited

55 Cancri: A Laboratory for Testing Numerous Conjectures about Planet Formation

Dimitris M. Christodoulou, Demosthenes Kazanas

Five planets are presently believed to orbit the primary star of 55 Cnc, but there exists a large 5 AU gap in their distribution between the two outermost planets. This gap has att…

astro-ph2008★ 28 cited

A novel method for measuring the extragalactic background light: Fermi application to the lobes of Fornax A

Markos Georganopoulos, Rita M. Sambruna, Demosthenes Kazanas +5

We describe a new method for measuring the extragalactic background light (EBL) through the detection of -ray inverse Compton (IC) emission due to scattering of the EBL photons…

astro-ph2008★ 67 cited

A multi-zone model for simulating the high energy variability of TeV blazars

Philip B. Graff, Markos Georganopoulos, Eric S. Perlman +1

We present a time-dependent multi-zone code for simulating the variability of Synchrotron-Self Compton (SSC) sources. The code adopts a multi-zone pipe geometry for the emission re…

astro-ph2008★ 4 cited

Cosmological Inflation: A Personal Perspective

Demosthenes Kazanas

We present a brief review of Cosmological Inflation from the personal perspective of the author who almost 30 years ago proposed a way of resolving the problem of Cosmological Hori…

astro-ph2007★ 16 cited

Light Echoes in Kerr Geometry: A Source of High Frequency QPOs from Random X-ray Bursts

Keigo Fukumura, Demosthenes Kazanas

We propose that high frequency quasi-periodic oscillations (HFQPOs) can be produced from randomly-formed X-ray bursts (flashes) by plasma interior to the ergosphere of a rapidly-ro…

astro-ph2007

Compton dragged supercritical piles: The GRB prompt and afterglow scenario

A. Mastichiadis, D. Kazanas

We examine the prompt and afterglow emission within the context of the Supercritical Pile model for GRBs. For this we have performed self-consistent calculations, by solving three…

astro-ph2007★ 18 cited

Mass Outflows from Dissipative Shocks in Hot Accretion Flows

Keigo Fukumura, Demosthenes Kazanas

We consider stationary, axisymmetric hydrodynamic accretion flows in Kerr geometry. As a plausible means of efficiently separating a small population of nonthermal particles from t…

astro-ph2007★ 23 cited

Simulations of the Poynting--Robertson Cosmic Battery in Resistive Accretion Disks

Dimitris M. Christodoulou, Ioannis Contopoulos, Demosthenes Kazanas

We describe the results of numerical "2.5--dimensional" MHD simulations of an initially unmagnetized disk model orbiting a central point--mass and responding to the continual gener…

astro-ph2007★ 7 cited

Exact Solutions of the Isothermal Lane--Emden Equation with Rotation and Implications for the Formation of Planets and Satellites

Dimitris M. Christodoulou, Demosthenes Kazanas

We have derived exact solutions of the isothermal Lane--Emden equation with and without rotation in a cylindrical geometry. The corresponding hydrostatic equilibria are most releva…

astro-ph2007★ 29 cited

Accretion Disk Illumination in Schwarzschild and Kerr Geometries: Fitting Formulae

Keigo Fukumura, Demosthenes Kazanas

We describe the methodology and compute the illumination of geometrically thin accretion disks around black holes of arbitrary spin parameter exposed to the radiation of a poin…

astro-ph2007

High Energy Variability Of Synchrotron-Self Compton Emitting Sources: Why One Zone Models Do Not Work And How We Can Fix It

Philip B. Graff, Markos Georganopoulos, Eric S. Perlman +1

With the anticipated launch of GLAST, the existing X-ray telescopes, and the enhanced capabilities of the new generation of TeV telescopes, developing tools for modeling the variab…

astro-ph2007★ 12 cited

Fourier-Resolved Spectroscopy of AGN using XMM-Newton data: I. The 3-10 keV band results

I. E. Papadakis, Z. Ioannou, D. Kazanas

We present the results from the Fourier Resolved Spectroscopy of archival XMM-Newton data of five AGN, namely, Mrk 766, NGC 3516, NGC 3783, NGC 4051 and Ark 564. This work suppleme…

astro-ph2006★ 1 cited

The "Supercritical Pile" GRB Model: Afterglows and GRB, XRR, XRF Unification

Demosthenes Kazanas, Apostolos Mastichiadis, Markos Georganopoulos

We present the general notions and observational consequences of the "Supercritical Pile" GRB model; the fundamental feature of this model is a detailed process for the conversion…

astro-ph2006★ 61 cited

Quasar X-ray jets: Gamma-ray diagnostics of the synchrotron and inverse Compton hypotheses, the case of 3C 273

Markos Georganopoulos, Eric S. Perlman, Demosthenes Kazanas +1

The process responsible for the Chandra-detected X-ray emission from the large scale jets of powerful quasars is a matter of ongoing debate. The two main contenders are external Co…

astro-ph2006★ 11 cited

Hubble Space Telescope Ultraviolet Spectroscopy of Fourteen Low-Redshift Quasars

Rajib Ganguly, Michael S. Brotherton, Nahum Arav +35

We present low-resolution ultraviolet spectra of 14 low redshift (z<0.8) quasars observed with HST/STIS as part of a Snap project to understand the relationship between quasar outf…

astro-ph2006★ 42 cited

The Cosmic Battery Revisited

Ioannis Contopoulos Demosthenes Kazanas Dimitris M. Christodoulou

We reinvestigate the generation and accumulation of magnetic flux in optically thin accretion flows around active gravitating objects. The source of the magnetic field is the azimu…

astro-ph2006★ 15 cited

Fourier resolved spectroscopy of 4U 1543-47 during the 2002 outburst

P. Reig, I. E. Papadakis, C. R. Shrader +1

We have obtained Fourier-resolved spectra of the black-hole binary 4U 1543-47 in the canonical states (high/soft, very high, intermediate and low/hard) observed in this source duri…

astro-ph2005

The Supercritical Pile Model for GRBs

A. Mastichiadis, D. Kazanas

We present the spectral and temporal radiative signatures expected within the "Supercritical Pile" model of Gamma Ray Bursts (GRB). This model is motivated by the need for a proces…

astro-ph2005★ 71 cited

Is the core of M87 the source of its TeV emission? Implications for unified schemes

Markos Georganopoulos, Eric S. Perlman, Demosthenes Kazanas

M87 has been recently shown to be a TeV source which is likely to be variable. Based on this, and on contemporaneous optical and X-ray monitoring, we argue that the source of the T…

astro-ph2005

How is the blazar GeV emission really produced?

Markos Georganopoulos, Eric Perlman, Demosthenes Kazanas +1

We show that the external Compton (EC) model for the production of the GeV emission in blazars makes specific predictions for the spectrum and variability of those blazars characte…

astro-ph2005★ 19 cited

Fourier Resolved Spectroscopy of the XMM-Newton Observations of MCG -6-30-15

I. E. Papadakis, D. Kazanas, A. Akylas

We study the Frequency Resolved Spectra of the Seyfert galaxy MCG -6-30-15 obtained during two recent XMM-Newton observations. Splitting the Fourier spectra in soft (<2 keV) and ha…

astro-ph2005★ 269 cited

Long-lag, Wide-Pulse Gamma-Ray Bursts

J. P. Norris, J. T. Bonnell, D. Kazanas +3

Currently, the best available probe of the early phase of gamma-ray burst (GRB) jet attributes is the prompt gamma-ray emission, in which several intrinsic and extrinsic variables…

astro-ph2005★ 25 cited

Bulk Comptonization of the Cosmic Microwave Background by Extragalactic Jets as a Probe of their Matter Content

Markos Georganopoulos, Demosthenes Kazanas, Eric Perlman +1

We propose a method for estimating the composition, i.e. the relative amounts of leptons and protons, of extragalactic jets which exhibit X-ray bright knots in their kpc scale jets…

astro-ph2004★ 65 cited

Witnessing the gradual slow-down of powerful extragalactic jets: The X-ray -- optical -- radio connection

Markos Georganopoulos, Demosthenes Kazanas

A puzzling feature of the {\it Chandra}--detected quasar jets is that their X-ray emission decreases faster along the jet than their radio emission, resulting to an outward increas…