Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and $\gamma$-ray emission

Emission of SN 1006 produced by accelerated cosmic rays

Berezhko, E.
Ksenofontov, L.
Völk, H.

December 2002

The nonlinear kinetic model of cosmic ray (CR) acceleration in supernova remnants (SNRs) is used to ...

Nonthermal emission from the reverse shock of the youngest Galactic supernova remnant G1.9+0.3

Brose, R.
Sushch, I.
Pohl, M.
Luken, K.J.
Filipovic, M.D.
Lin, R.

January 2019

International audienceContext. The youngest Galactic supernova remnant G1.9+0.3 is an interesting ta...

The supernova remnant SN 1006 as a Galactic particle accelerator

Giuffrida, Roberta
Miceli, Marco
Caprioli, Damiano
Decourchelle, Anne
Vink, Jacco
Orlando, Salvatore
Bocchino, Fabrizio
Greco, Emanuele
Peres, Giovanni

August 2022

The origin of cosmic rays is a pivotal open issue of high-energy astrophysics. Supernova remnants a...

Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and $\gamma$-ray emission

Miceli, Marco
Orlando, Salvatore
Pereira, Victor
Acero, Fabio
Katsuda, Satoru
Decourchelle, Anne
Winkler, Frank P.
Bonito, Rosaria
Reale, Fabio
Peres, Giovanni
Li, Jiangtao
Dubner, Gloria

January 2016

International audienceContext. The supernova remnant SN 1006 is a source of high-energyparticles and...

Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and

M. Miceli
S. Orlando
V. Pereira
F. Acero
S. Katsuda
A. Decourchelle
F. P. Winkler
R. Bonito
F. Reale
G. Peres
J. Li
G. Dubner

August 2016

Context. The supernova remnant SN 1006 is a source of high-energy particles and its southw...

SHOCK-cloud interaction and particle acceleration in the southwestern limb of sn 1006

MICELI, Marco
Acero, F.
Dubner, G.
Decourchelle, A.
Orlando, S.
Bocchino, F.

January 2014

The supernova remnant SN 1006 is a powerful source of high-energy particles and evolves in a relativ...

Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and γ-ray emission

MICELI, Marco
Orlando, S.
Pereira, V.
Acero, F.
Katsuda, S.
Decourchelle, A.
Winkler, F.
BONITO, Rosaria
REALE, Fabio
PERES, Giovanni
Li, J.
Dubner, G.

January 2016

Context. The supernova remnant SN 1006 is a source of high-energy particles and its southwestern lim...

Shock-Cloud Interaction and Particle Acceleration in the Southwestern Limb of SN 1006

Miceli, M.
Acero, F.
Dubner, Gloria Mabel
Decourchelle, A.
Orlando, S.
Bocchino, F.

February 2014

The supernova remnant SN 1006 is a powerful source of high-energy particles and evolves in a relativ...

Gamma-ray models for SN 1006 using different astronomical parameters

Ksenofontov, L.
Berezhko, E.
Völk, H.

July 2004

We use nonlinear kinetic theory of cosmic ray acceleration in supernova remnants to study the proper...

Dependence of the gamma-ray emission from SN 1006 on the astronomical parameters

Ksenofontov, L.T.
Berezhko, E.G.
Völk, H.J.

January 2005

We use nonlinear theory to study the remnant dynamics and the particle acceleration as well as the p...

Dependence of the Gamma-Ray Emission from SN 1006 on the Astronomical Parameters

Ksenofontov, L.
Berezhko, E.
Völk, H.

January 2005

We use nonlinear kinetic theory to study cosmic ray acceleration and the properties of the nontherma...

Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006

MICELI, Marco
Bocchino, F.
Iakubovskyi, D.
Orlando, S.
Telezhinsky, I.
Kirsch, M. G. F.
Petruk, O.
Dubner, G.
Castelletti, G.

January 2009

Context. Efficient particle acceleration can modify the structure of supernova remnants. We present ...

The gas density around SN 1006

F. Acero
J. Ballet
A. Decourchelle

October 2007

Context.The density of the ambient medium where the supernova remnant evolves is a relevant paramete...

X-Ray observations of SN 1006 with INTEGRAL

Kalemci, Emrah
Reynolds, Stephen
Boggs, Steven E.
Lund, Niels
Chenevez, Jerome
Renaud, Matthieu
Rho, J.

June 2006

The remnant of the supernova of 1006 AD, the remnant first showing evidence for the presence of X-ra...

33RD INTERNATIONAL COSMIC RAY CONFERENCE, RIO DE JANEIRO 2013 THE ASTROPARTICLE PHYSICS CONFERENCE

January 2016

Abstract: The properties of the Galactic supernova remnant (SNR) SN 1006 are theoretically re-analyz...

Emission of SN 1006 produced by accelerated cosmic rays

Berezhko, E.
Ksenofontov, L.
Völk, H.

December 2002

The nonlinear kinetic model of cosmic ray (CR) acceleration in supernova remnants (SNRs) is used to ...

Nonthermal emission from the reverse shock of the youngest Galactic supernova remnant G1.9+0.3

Brose, R.
Sushch, I.
Pohl, M.
Luken, K.J.
Filipovic, M.D.
Lin, R.

January 2019

International audienceContext. The youngest Galactic supernova remnant G1.9+0.3 is an interesting ta...

The supernova remnant SN 1006 as a Galactic particle accelerator

Giuffrida, Roberta
Miceli, Marco
Caprioli, Damiano
Decourchelle, Anne
Vink, Jacco
Orlando, Salvatore
Bocchino, Fabrizio
Greco, Emanuele
Peres, Giovanni

August 2022

The origin of cosmic rays is a pivotal open issue of high-energy astrophysics. Supernova remnants a...

Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and $\gamma$-ray emission

Miceli, Marco
Orlando, Salvatore
Pereira, Victor
Acero, Fabio
Katsuda, Satoru
Decourchelle, Anne
Winkler, Frank P.
Bonito, Rosaria
Reale, Fabio
Peres, Giovanni
Li, Jiangtao
Dubner, Gloria

January 2016

International audienceContext. The supernova remnant SN 1006 is a source of high-energyparticles and...

Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and

M. Miceli
S. Orlando
V. Pereira
F. Acero
S. Katsuda
A. Decourchelle
F. P. Winkler
R. Bonito
F. Reale
G. Peres
J. Li
G. Dubner

August 2016

Context. The supernova remnant SN 1006 is a source of high-energy particles and its southw...

SHOCK-cloud interaction and particle acceleration in the southwestern limb of sn 1006

MICELI, Marco
Acero, F.
Dubner, G.
Decourchelle, A.
Orlando, S.
Bocchino, F.

January 2014

The supernova remnant SN 1006 is a powerful source of high-energy particles and evolves in a relativ...

Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and γ-ray emission

MICELI, Marco
Orlando, S.
Pereira, V.
Acero, F.
Katsuda, S.
Decourchelle, A.
Winkler, F.
BONITO, Rosaria
REALE, Fabio
PERES, Giovanni
Li, J.
Dubner, G.

January 2016

Context. The supernova remnant SN 1006 is a source of high-energy particles and its southwestern lim...

Shock-Cloud Interaction and Particle Acceleration in the Southwestern Limb of SN 1006

Miceli, M.
Acero, F.
Dubner, Gloria Mabel
Decourchelle, A.
Orlando, S.
Bocchino, F.

February 2014

The supernova remnant SN 1006 is a powerful source of high-energy particles and evolves in a relativ...

Gamma-ray models for SN 1006 using different astronomical parameters

Ksenofontov, L.
Berezhko, E.
Völk, H.

July 2004

We use nonlinear kinetic theory of cosmic ray acceleration in supernova remnants to study the proper...

Dependence of the gamma-ray emission from SN 1006 on the astronomical parameters

Ksenofontov, L.T.
Berezhko, E.G.
Völk, H.J.

January 2005

We use nonlinear theory to study the remnant dynamics and the particle acceleration as well as the p...

Dependence of the Gamma-Ray Emission from SN 1006 on the Astronomical Parameters

Ksenofontov, L.
Berezhko, E.
Völk, H.

January 2005

We use nonlinear kinetic theory to study cosmic ray acceleration and the properties of the nontherma...

Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006

MICELI, Marco
Bocchino, F.
Iakubovskyi, D.
Orlando, S.
Telezhinsky, I.
Kirsch, M. G. F.
Petruk, O.
Dubner, G.
Castelletti, G.

January 2009

Context. Efficient particle acceleration can modify the structure of supernova remnants. We present ...

The gas density around SN 1006

F. Acero
J. Ballet
A. Decourchelle

October 2007

Context.The density of the ambient medium where the supernova remnant evolves is a relevant paramete...

X-Ray observations of SN 1006 with INTEGRAL

Kalemci, Emrah
Reynolds, Stephen
Boggs, Steven E.
Lund, Niels
Chenevez, Jerome
Renaud, Matthieu
Rho, J.

June 2006

The remnant of the supernova of 1006 AD, the remnant first showing evidence for the presence of X-ra...

33RD INTERNATIONAL COSMIC RAY CONFERENCE, RIO DE JANEIRO 2013 THE ASTROPARTICLE PHYSICS CONFERENCE

January 2016

Abstract: The properties of the Galactic supernova remnant (SNR) SN 1006 are theoretically re-analyz...

Emission of SN 1006 produced by accelerated cosmic rays

Berezhko, E.
Ksenofontov, L.
Völk, H.

December 2002

The nonlinear kinetic model of cosmic ray (CR) acceleration in supernova remnants (SNRs) is used to ...

Nonthermal emission from the reverse shock of the youngest Galactic supernova remnant G1.9+0.3

Brose, R.
Sushch, I.
Pohl, M.
Luken, K.J.
Filipovic, M.D.
Lin, R.

January 2019

International audienceContext. The youngest Galactic supernova remnant G1.9+0.3 is an interesting ta...

The supernova remnant SN 1006 as a Galactic particle accelerator

Giuffrida, Roberta
Miceli, Marco
Caprioli, Damiano
Decourchelle, Anne
Vink, Jacco
Orlando, Salvatore
Bocchino, Fabrizio
Greco, Emanuele
Peres, Giovanni

August 2022

The origin of cosmic rays is a pivotal open issue of high-energy astrophysics. Supernova remnants a...

Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and $\gamma$-ray emission

Abstract

Extracted data

Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and $\gamma$-ray emission

Abstract

Extracted data

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