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IRAS 15099−5856: Remarkable Mid-Infrared Source with Prominent Crystalline Silicate Emission Embedded in the Supernova Remnant MSH15−52
(The Astrophysical Journal, 2011)
The neutral gas environment of the young supernova remnant SN 1006 (G327.6+14.6)
(EDP Sciences, 2002-06)
Using the Australia Telescope Compact Array, we have carried out a survey of the H i emission in the direction of the bilateral supernova remnant (SNR) SN 1006 (G327.6+14.6). The angular resolution of the data is 4.07×3.00, ...
G51.04+0.07 and its environment: Identification of a new Galactic supernova remnant at low radio frequencies
(EDP Sciences, 2018-04)
We have identified a new supernova remnant (SNR), G51.04+0.07, using observations at 74 MHz from the Very Large Array Low-Frequency Sky Survey Redux (VLSSr). Earlier, higher frequency radio continuum, recombination line, ...
GeV Emission in the Region of the Supernova Remnant G51.26+0.11
(2021-11-02)
The supernova remnant G51.26+0.11 was recently discovered and little is known about its properties and environment. Using data from the Fermi Large Area Telescope we study the GeV emission seen in the direction of G51.26+0.11 ...
XMM-Newton detection of the supernova remnant G304.6+0.1 (Kes 17)
(Edp Sciences, 2010)
The Supernova Remnant W44: confirmations and challenges for cosmic-ray acceleration
(Edp Sciences, 2014-03)
The middle-aged supernova remnant (SNR) W44 has recently attracted attention because of its relevance regarding the origin of Galactic cosmic-rays. The gamma-ray missions AGILE and Fermi have established, for the first ...
A new study of the supernova remnant G344.7-0.1 located in the vicinity of the unidentified TeV source HESS J1702-420
(EDP Sciences, 2011-07)
Context. The identification of counterparts of dark gamma-ray sources adds greatly to our understanding of their underlying astrophysical processes.
Aims. We investigate the physical properties of the supernova remnant ...
The Cherenkov Telescope Array potential for the study of young supernova remnants
(Elsevier Science, 2015-03)
Supernova remnants (SNRs) are among the most important targets for γ-ray observatories. Being prominent non-thermal sources, they are very likely responsible for the acceleration of the bulk of Galactic cosmic rays (CRs). ...
Interstellar Gas and X-rays toward the Young Supernova Remnant RCW 86; Pursuit of the Origin of the Thermal and Non-thermal X-ray
(Elsevier, 2017-09)
We have analyzed the atomic and molecular gas using the 21 cm HI and 2.6/1.3 mm CO emissions toward the young supernova remnant (SNR) RCW 86 in order to identify the interstellar medium with which the shock waves of the ...