NewEvery arXiv paper, its researchers & institutions — mapped.
papers

Publications (29)

astro-ph.HE2015

CTA Contributions to the 34th International Cosmic Ray Conference (ICRC2015)

The CTA Consortium, :, A. Abchiche +1305

astro-ph2005

The nature of the X-ray halo of the plerion G21.5-0.9 unveiled by XMM-Newton and Chandra

F. Bocchino, E. van der Swaluw, R. Chevalier +1

astro-ph.HE2012

Collisionless shocks in a partially ionized medium: I. Neutral return flux and its effects on acceleration of test particles

P. Blasi, G. Morlino, R. Bandiera +2

astro-ph.HE2016

Unveiling the Magnetic Structure of VHE SNRs/PWNe with XIPE, the X-ray Imaging-Polarimetry Satellite

E. de Ona Wilhelmi, J. Vink, A. Bykov +6

astro-ph.HE2012

Collisionless shock in a partially ionized medium. II. Balmer emission

G. Morlino, R. Bandiera, P. Blasi +1

astro-ph.HE2017

Discovery of a Synchrotron Bubble Associated with PSR J1015-5719

C. -Y. Ng, R. Bandiera, R. W. Hunstead +1

astro-ph.HE2010

XMM-Newton and Suzaku detection of an X-ray emitting shell around the pulsar wind nebula G54.1+0.3

F. Bocchino, R. Bandiera, J. Gelfand

astro-ph2004

Analytic Solutions for the Evolution of Radiative Supernova Remnants

R. Bandiera, O. Petruk

astro-ph.HE2016

Contributions of the Cherenkov Telescope Array (CTA) to the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016)

The CTA Consortium, :, A. Abchiche +1387

astro-ph.HE2013

CTA contributions to the 33rd International Cosmic Ray Conference (ICRC2013)

The CTA Consortium, :, O. Abril +1102

astro-ph1996

The Supernova Remnant G11.2-0.3 and its central Pulsar

R. Bandiera, F. Pacini, M. Salvati

astro-ph.HE2013

Cosmic Ray acceleration and Balmer emission from SNR 0509-67.5

G. Morlino, P. Blasi, R. Bandiera +1

astro-ph.GA2012

Infrared imaging and polarimetric observations of the pulsar wind nebula in SNR G21.5-0.9

A. Zajczyk, Y. A. Gallant, P. Slane +6

astro-ph2006

Influence of Thermalisation on Electron Injection in Supernova Remnant Shocks

O. Petruk, R. Bandiera

astro-ph2002

BeppoSAX observation of the composite remnant G327.1-1.1

F. Bocchino, R. Bandiera

astro-ph.HE2017

Cherenkov Telescope Array Contributions to the 35th International Cosmic Ray Conference (ICRC2017)

F. Acero, B. S. Acharya, V. Acín Portella +1137

astro-ph2000

A model for the spatial distribution of relativistic electrons in the Crab Nebula

E. Amato, M. Salvati, R. Bandiera +2

astro-ph.HE2019

The dust content of the Crab Nebula

I. De Looze, M. J. Barlow, R. Bandiera +7

astro-ph.HE2013

Collisionless shocks in a partially ionized medium: III. Efficient cosmic ray acceleration

G. Morlino, P. Blasi, R. Bandiera +2

astro-ph2002

A catalogue of damped Lyman alpha absorption systems and radio flux densities of the background quasars

S. J. Curran, J. K. Webb, M. T. Murphy +3

astro-ph.HE2017

Modeling the effect of small-scale magnetic turbulence on the X-ray properties of Pulsar Wind Nebulae

N. Bucciantini, R. Bandiera, B. Olmi +1

astro-ph.HE2014

Cosmic Ray acceleration and Balmer emission from RCW 86 (G315.4-2.3)

G. Morlino, P. Blasi, R. Bandiera +1

astro-ph.HE2009

A statistical approach to radio emission from shell-type SNRs. I. Basic ideas, techniques, and first results

R. Bandiera, O. Petruk

astro-ph2004

The effects of spin-down on the structure and evolution of pulsar wind nebulae

N. Bucciantini, R. Bandiera, J. M. Blondin +2

astro-ph2003

The X-ray Halo of G21.5-0.9

R. Bandiera, F. Bocchino

astro-ph.HE2017

Radio polarization maps of shell-type SNRs II. Sedov models with evolution of turbulent magnetic field

O. Petruk, R. Bandiera, V. Beshley +2

astro-ph2004

Magnetic Rayleigh-Taylor instability for Pulsar Wind Nebulae in expanding Supernova Remnants

N. Bucciantini, E. Amato, R. Bandiera +2

astro-ph.HE2013

Broad Balmer line emission and cosmic ray acceleration efficiency in supernova remnant shocks

G. Morlino, P. Blasi, R. Bandiera +1

astro-ph2002

BeppoSAX observations of the young pulsar in the Kes 75 Supernova Remnant

S. Mereghetti, R. Bandiera, F. Bocchino +1