English
Related papers

Related papers: Spectral Properties of M87 Using Two-Component Flo…

200 papers

We consider the synchrotron spectrum produced by mildly-to-highly relativistic collisionless shocks. Simple analytic formulae are derived for the break frequencies (peak frequency, self-absorption frequency, synchrotron and inverse Compton…

High Energy Astrophysical Phenomena · Physics 2024-12-03 Gilad Sadeh

We study Compton upscattering of low-frequency photons in a converging flow of thermal plasma. The photons escape diffusively and electron scattering is the dominant source of opacity. We solve numerically and approximately analytically the…

Astrophysics · Physics 2009-10-30 L. Titarchuk , A. Mastichiadis , N. D. Kylafis

We explore the evolution of the emissions by accelerated electrons in shocked shells driven by jets in active galactic nuclei (AGNs). Focusing on powerful sources which host luminous quasars, we evaluated the broadband emission spectra by…

High Energy Astrophysical Phenomena · Physics 2011-03-18 H. Ito , M. Kino , N. Kawakatu , S. yamada

In the present paper an alternative theoretical interpretation to the generally assumed thermal emission models of the observed X-ray spectrum of isolated pulsar RX J0420.0-5022 is presented. It is well known that the distribution function…

High Energy Astrophysical Phenomena · Physics 2013-04-09 Nino Chkheidze , Iurii Babyk

We propose a new approximation for the cyclo-synchrotron emissivity of a single electron. In the second part of this work, we discuss a simple application for our approximation, and investigate the heating of electrons through the…

Astrophysics · Physics 2009-11-11 K. Katarzynski , G. Ghisellini , R. Svensson , J. Gracia

The discovery of diffuse synchrotron radio emission and, more recently, of the hard X-ray (HXR) tails have triggered a growing interest about non-thermal phenomena in galaxy clusters. After a brief review of the most important evidences for…

Astrophysics · Physics 2009-11-10 Gianfranco Brunetti

We have examined the hypothesis that the majority of the diffuse EUV flux in the Coma cluster is due to inverse Compton scattering of low energy cosmic ray electrons (0.16 < epsilon < 0.31 GeV) against the 3K black-body background. We…

Astrophysics · Physics 2009-10-30 Stuart Bowyer , Thomas W. Berghoefer

We present hard X-ray observations of the nearby radio galaxy M87 and the core of the Virgo cluster using the Rossi X-ray Timing Explorer. These are the first hard X-ray observations of M87 not affected by contamination from the nearby…

Astrophysics · Physics 2015-09-16 C. S. Reynolds , S. Heinz , A. C. Fabian , M. C. Begelman

Non dispersive electronic Rydberg wave packets may be created in atoms illuminated by a microwave field of circular polarization. We discuss the spontaneous emission from such states and show that the elastic incoherent component (occuring…

Quantum Physics · Physics 2009-10-31 Dominique Delande , Jakub Zakrzewski

We present a model for electron- and neutrino-scattering off nucleons and nuclei focussing on the quasielastic and resonance region. The lepton-nucleon reaction is described within a relativistic formalism that includes, besides…

Nuclear Theory · Physics 2009-04-03 T. Leitner , O. Buss , L. Alvarez-Ruso , U. Mosel

We study how the spectral properties of resonance fluorescence propagate through a two-atom system. Within the weak-driving-field approximation we find that, as we go from one atom to the next, the power spectrum exhibits both sub-natural…

Atomic Physics · Physics 2009-10-31 R. Marani , M. Artoni

Gamma-ray data from Fermi-LAT reveal a bi-lobular structure extending up to 50 degrees above and below the galactic centre, which presumably originated in some form of energy release there less than a few million years ago. It has been…

High Energy Astrophysical Phenomena · Physics 2011-08-26 Philipp Mertsch , Subir Sarkar

A growing number of both galactic and extragalactic supernova remnants show non-thermal (non-plerionic) emission in the X-ray band. New synchrotron models, realized as SRESC and SRCUT in XSPEC 11, which use the radio spectral index and flux…

Astrophysics · Physics 2009-11-06 Kristy Dyer , Stephen Reynolds , Kazik Borkowski , Rob Petre

We develop a semiclassical theory for the spectral rigidity of non-hydrogenic Rydberg atoms in electric fields and evaluate the significant deviations from the well-known Poissonian behaviour in the hydrogenic case. The resulting formula is…

chao-dyn · Physics 2009-10-31 P. N. Walker , T. S. Monteiro

We summarize HST observations of the M87 jet, concentrating on polarimetry and spectral index maps, and compare its optical and radio structures. The evidence now supports a stratified model for the structure of the jet, whereby…

Astrophysics · Physics 2007-05-23 Eric Perlman , William Sparks , John Biretta , Duccio Macchetto , J. Patrick Leahy

We study the emission of neutrinos, resulting from the scattering of electrons off magnetic flux tubes (fluxoids) in the neutron star cores with superfluid (superconducting) protons. In the absence of proton superfluidity (T> T_{cp}), this…

Astrophysics · Physics 2007-05-23 A. D. Kaminker , D. G. Yakovlev , P. Haensel

We consider two-nucleon scattering close to threshold. Partial-wave amplitudes are obtained by an analytic extrapolation of subthreshold reaction amplitudes calculated in a relativistic formulation of chiral perturbation theory. The…

Nuclear Theory · Physics 2015-06-12 A. M. Gasparyan , M. F. M. Lutz , E. Epelbaum

We discuss the observational phenomenology of Seyferts from the point of view of the disk model, and argue that the spectral variability may be related to geometrical changes of the cold matter which provides a source of seed photons for…

Astrophysics · Physics 2007-05-23 P. Magdziarz

We derive the formula of the complex Doppler shift in a two-dimensional, dispersive metamaterial and we show that a moving, monochromatic radiation source generates multiple frequency modes. The role of the group velocity is stressed and…

Optics · Physics 2015-03-26 David Ziemkiewicz , Sylwia Zielińska-Raczyńska

We discuss the synchrotron emission of fast cooling electrons in shocks. The fast cooling electrons behind the shocks can generate a position-dependent inhomogeneous electron distribution if they do not have enough time to mix…

High Energy Astrophysical Phenomena · Physics 2017-04-27 Xiao-hong Zhao , Jin-ming Bai
‹ Prev 1 8 9 10 Next ›