Results 131 to 140 of about 197,763 (248)
Constraints on the cosmic ray diffusion coefficient in the W28 region from gamma-ray observations
GeV and TeV gamma rays have been detected from the supernova remnant W28 and its surroundings. Such emission correlates quite well with the position of dense and massive molecular clouds and thus it is often interpreted as the result of hadronic cosmic ...
Aharonian, F. A. +3 more
core +1 more source
Searching for galactic cosmic ray pevatrons with multi-TeV gamma rays and neutrinos
The recent HESS detections of supernova remnant shells in TeV gamma-rays confirm the theoretical predictions that supernova remnants can operate as powerful cosmic ray accelerators.
Aharonian F. A. +4 more
core +1 more source
JWST observations of the young Galactic supernova remnant Cassiopeia A revealed an unexpected structure seen as a green emission feature in colored composite MIRI F1130W and F1280W images—hence dubbed the Green Monster—that stretches across the central ...
Ilse De Looze +29 more
doaj +1 more source
Circinus X-1: survivor of a highly asymmetric supernova
We have analyzed the kinematical parameters of Cir X-1 to constrain the nature of its companion star, the eccentricity of the binary and the pre-supernova parameter space.
Case +22 more
core +2 more sources
A population of isolated hard X-ray sources near the supernova remnant Kes 69
Recent X-ray observations of the supernova remnant IC443 interacting with molecular clouds have shown the presence of a new population of hard X-ray sources related to the remnant itself, which has been interpreted in terms of fast ejecta fragment ...
A. M. Bykov +57 more
core +1 more source
ROLE OF EJECTA CLUMPING AND BACK-REACTION OF ACCELERATED COSMIC RAYS IN THE EVOLUTION OF TYPE Ia SUPERNOVA REMNANTS [PDF]
Orlando S +9 more
openalex +1 more source
The circumstellar medium of the peculiar supernova SN1997ab
We report the detection of the slow moving wind into which the compact supernova remnant SN 1997ab is expanding. Echelle spectroscopy provides clear evidence for a well resolved narrow (Full Width at Zero Intensity, FWZI ~ 180 km/s) P-Cygni profile, both
Cid-Fernandes, Roberto +5 more
core +1 more source
New candidate radio supernova remnants detected in the GLEAM survey over 345° <l< 60°, 180° <l< 240° [PDF]
N. Hurley‐Walker +20 more
openalex +1 more source
The Distance to the S147 Supernova Remnant
In the absence of a parallax distance to a pulsar or a surviving binary in a supernova remnant (SNR), distances to Galactic SNRs are generally very uncertain.
C. S. Kochanek +2 more
doaj +1 more source
The light emission (“glow”) of cold dusty plasma of the remnant of SN 1987A was confirmed by the Hubble Space Telescope observations on 7th January, 1995.
D. N. Doikov, S. M. Andrievsky
doaj +1 more source

