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相关论文: Supernova remnants and gamma-ray sources

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Particle acceleration in the dynamically evolving environment of Supernova Remnants is discussed in the framework of a genuinely time-dependent nonlinear theory, assuming spherical symmetry. As a consequence the dependence of injection on…

天体物理学 · 物理学 2007-05-23 H. J. Voelk

Supernova remnants are beautiful astronomical objects that are also of high scientific interest, because they provide insights into supernova explosion mechanisms, and because they are the likely sources of Galactic cosmic rays. X-ray…

高能天体物理现象 · 物理学 2012-01-05 Jacco Vink

The gamma-ray observations of molecular clouds associated with supernova remnants are considered one of the most promising ways to search for a solution of the problem of cosmic ray origin. Here we briefly review the status of the field,…

高能天体物理现象 · 物理学 2015-12-16 S. Gabici , J. Krause , G. Morlino , L. Nava

Supernova remnants (SNRs) are widely believed to be the principal source of galactic cosmic rays. Such energetic particles can produce gamma-rays and lower energy photons via interactions with the ambient plasma. In this paper, we present…

In the past few years, gamma-ray astronomy has entered a golden age thanks to two major breakthroughs: Cherenkov telescopes on the ground and the Large Area Telescope (LAT) onboard the Fermi satellite. The sample of supernova remnants…

高能天体物理现象 · 物理学 2015-10-06 John W. Hewitt , Marianne Lemoine-Goumard

Supernova remnants (SNRs) are widely considered the most likely source of cosmic rays below the knee ($10^{15}$ eV). Studies of GeV and TeV gamma-ray emission in the vicinity of SNRs, in combination with multi-wavelength observations, can…

高能天体物理现象 · 物理学 2019-08-13 Amanda Weinstein

While the definitive detection of gamma-rays from known supernova remnants (SNRs) remains elusive, the collection of unidentified EGRET sources that may be associated with SNRs has motivated recent modelling of TeV emission from these…

天体物理学 · 物理学 2007-05-23 Matthew G. Baring , Donald C. Ellison , Isabelle Grenier

Supernova remnants are widely believed to be a principal source of galactic cosmic rays, produced by diffusive shock acceleration in the environs of the remnant's expanding shock. This review discusses recent modelling of how such energetic…

天体物理学 · 物理学 2007-05-23 Matthew G. Baring

Galactic cosmic rays are believed to be accelerated at supernova remnant shocks. Gamma-ray observations of both supernova remnants and associated molecular clouds have been used in several occasions to test (so far quite successfully) this…

高能天体物理现象 · 物理学 2017-08-09 Stefano Gabici

Recent results obtained with gamma-ray satellites have established supernova remnants as accelerators of GeV hadronic cosmic rays. In such processes, CRs accelerated in SNR shocks interact with particles from gas clouds in their…

高能天体物理现象 · 物理学 2020-08-14 Emma de Ona Wilhelmi , Iurii Sushch , Robert Brose , Enrique Mestre , Yang Su , Roberta Zanin

The origin of cosmic rays is one of the long-standing mysteries in physics and astrophysics. Simple arguments suggest that a scenario of supernova remnants (SNRs) in the Milky Way as the dominant sources for the cosmic ray population below…

高能天体物理现象 · 物理学 2016-06-01 Julia Becker Tjus , Björn Eichmann , Mike Kroll , Nils Nierstenhöfer

Supernova remnants (SNRs) are the prime candidates for the acceleration of the Galactic Cosmic Rays. Tracers for interactions of Cosmic Rays with ambient material are gamma rays at TeV energies, which can be observed with ground based…

高能天体物理现象 · 物理学 2019-08-14 Nukri Komin

Galactic cosmic rays are believed to be accelerated at supernova remnant shocks. Though very popular and robust, this conjecture still needs a conclusive proof. The strongest support to this idea is probably the fact that supernova remnants…

高能天体物理现象 · 物理学 2015-06-15 P. Cristofari , S. Gabici , S. Casanova , R. Terrier , E. Parizot

This is a report on the findings of the SNR/cosmic-ray working group for the white paper on the status and future of ground-based gamma-ray astronomy. The white paper is an APS commissioned document, and the overall version has also been…

Despite tantalizing evidence that supernova remnants (SNRs) are the source of Galactic cosmic rays (CRs), including the recent detection of a spectral signature of hadronic gamma-ray emission from two SNRs, their origin in aggregate remains…

高能天体物理现象 · 物理学 2019-08-13 T. J. Brandt , F. Acero , F. de Palma , J. W. Hewitt , M. Renaud

It is shown that the radio and gamma-ray emission observed from newly-found "GeV-bright" supernova remnants (SNRs) can be explained by a model, in which a shocked cloud and shock-accelerated cosmic rays (CRs) frozen in it are simultaneously…

高能天体物理现象 · 物理学 2015-05-19 Yasunobu Uchiyama , Roger Blandford , Stefan Funk , Hiroyasu Tajima , Takaaki Tanaka

While supernova remnants (SNRs) are widely thought to be powerful accelerators, evidence comes largely from a small number of well-studied cases. Here we systematically determine the gamma-ray emission from all known Galactic SNRs,…

高能天体物理现象 · 物理学 2019-08-13 J. W. Hewitt , F. Acero , T. J. Brandt , J. Cohen , F. de Palma , F. Giordano

We analyze the results of recent measurements of Galactic cosmic ray (GCRs) energy spectra and the spectra of nonthermal emission from supernova remnants (SNRs) in order to determine their consistency with GCR origin in SNRs. It is shown…

高能天体物理现象 · 物理学 2014-12-30 E. G. Berezhko

In this paper we briefly comment on the observational status of the possible physical association between unidentified EGRET sources and supernova remnants (SNRs) in our Galaxy. We draw upon recent results presented in the review by Torres…

天体物理学 · 物理学 2009-11-10 Diego F. Torres , Thomas M. Dame , Gustavo E. Romero

Increasing observational evidence gathered especially in X-rays and gamma-rays during the course of the last few years support the notion that Supernova remnants (SNRs) are Galactic particle accelerators up to energies close to the ``knee''…

天体物理学 · 物理学 2008-11-26 S. Funk