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A joint spectro-imaging analysis of the XMM-Newton and HESS observations of the supernova remnant RX J1713.7-3946
(EDP Sciences, 2008-12)
Context. The supernova remnant (SNR) RX J1713.7-3946 (also known as G347.3-0.5) is part of the class of remnants dominated by synchrotron emission in X-rays. It is also one of the few shell-type SNRs observed at TeV energies ...
On the origin of the jet-like radio/X-ray morphology of G290.1-0.8
(EDP Sciences, 2012-10)
Context. The origin and evolution of supernova remnants of the mixed-morphology class is not well understood. Several remnants present distorted radio or X-ray shells with jet-like structures. G290.1-0.8 (MSH 11-61A) belongs ...
Mass loss from the progenitor of SN 1006?
(Universidad Nacional Autónoma de México. Instituto de Astronomía, 2008)
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, ...
Proton and Hydrogen Transport through Hydrogen Environments: Ionization and Stripping
(IOP Publishing, 2020-12-23)
Data are presented over a wide range of impact energies describing the ionization or stripping probability, projectile energy loss, and ejected electron and recoiling target energies and angles for proton and hydrogen ...
Natal molecular cloud of SNR Kes 41. Complete characterisation
(EDP Sciences, 2018-11)
Using high-resolution data of the 12CO and 13CO (J = 1-0) line emission from the Mopra Southern Galactic Plane CO Survey in conjunction with neutral hydrogen observations from the Southern Galactic Plane Survey (SGPS) and ...
Unidentified γ-ray emission towards the SNR Kes 41 revisited
(EDP Sciences, 2018-11)
Kes 41 is one of the Galactic supernova remnants (SNRs) that are proposed to be physically linked to γ-ray emission at GeV energies. The nature of the γ-ray photons has been explained, but inconclusively, as hadronic ...
Searches for continuous gravitational waves from nine young supernova remnants
(IOP Publishing, 2015-10)
science data run. The targets were nine young supernova remnants not associated with pulsars; eight of the remnants are associated with non-pulsing suspected neutron stars. One target’s parameters are uncertain enough to ...
Non-thermal emission resulting from a supernova explosion inside an extragalactic jet
(EDP Sciences, 2019-02)
Context. Core-collapse supernovae are found in galaxies with ongoing star-formation. In a starburst galaxy hosting an active galactic nucleus with a relativistic jet, supernovae can take place inside the jet. The collision ...
The electron-capture origin of supernova 2018zd
(Nature Research, 2021-09-21)
In the transitional mass range (~8?10 solar masses) between white dwarf formation and iron core-collapse supernovae, stars are expected to produce an electron-capture supernova. Theoretically, these progenitors are thought ...