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The gigaelectronvolt counterpart of ver j2019+407 in the northern shell of the supernova remnant g78.2+2.1 (γ cygni)
(2016-07)
Analysis of gamma-ray emission from the supernova remnant G78.2+2.1 (γ Cygni) with 7.2 years of cumulative data from the Fermi Large Area Telescope shows a distinct hard, bright, and extended component to the north of the ...
The gigaelectronvolt counterpart of ver j2019+407 in the northern shell of the supernova remnant g78.2+2.1 (γ cygni)
(2016-07)
Analysis of gamma-ray emission from the supernova remnant G78.2+2.1 (γ Cygni) with 7.2 years of cumulative data from the Fermi Large Area Telescope shows a distinct hard, bright, and extended component to the north of the ...
Asymmetries in the Expansion and Emission from Young Supernova Remnants
(IOP Publishing, 2011-01)
We present two-dimensional and three-dimensional numerical simulations of asymmetric young supernova remnants (SNRs) carried out with the hydrodynamical code YGUAZÚ, aiming to quantitatively assess the role of different ...
A blowout numerical model for the supernova remnant G352.7-0.1
(Oxford University Press, 2014-01-08)
We present 3D hydrodynamical simulations of the Galactic supernova remnant G352.7−0.1. This remnant is peculiar for having a shell-like inner ring structure and an outer arc in radio observations. In our model, the supernova ...
Cassiopeia A Supernova Remnant
(Spitzer Space Telescope, 2016)
Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant
(Institute of Physics Publishing, 2011-02)
Supernova remnants (SNRs) have long been assumed to be the source of cosmic rays (CRs) up to the "knee" of the CR spectrum at 1015 eV, accelerating particles to relativistic energies in their blast waves by the process of ...
Origin of the bilateral structure of the supernova remnant G296.5+10
(Oxford University Press, 2017-08-14)
In this work, we have modelled the supernova remnant (SNR) G296.5+10, by means of 3D magnetohydrodynamics (MHD) simulations. This remnant belongs to the bilateral SNR group and has an additional striking feature: the ...
Isolated X-ray Infrared sources in the region of interaction of the Supernova Remnant IC443 with a molecular cloud
(IOP Publishing, 2008-12)
The nature of the extended hard X-ray source XMMU J061804.3+222732 and its surroundings is investigated using XMM-Newton, Chandra, and Spitzer observations. This source is located in an interaction region of the IC 443 ...
The physical connection between G337.2+0.1 and AX J1635.9-4719
(Società Astronomica Italiana, 2005-12)
We present evidence supporting a SNR origin for the radio source G337.2+0.1, which was discovered in the MOST 843-MHz radio survey. The radio source is spatially coincident with the unidentified ASCA source AX J1635.9-4719. ...