Results 151 to 160 of about 201,431 (246)
Nonthermal Signatures of Radiative Supernova Remnants
The end of supernova remnant (SNR) evolution is characterized by a so-called “radiative” stage, in which efficient cooling of the hot bubble inside the forward shock slows expansion, leading to eventual shock breakup.
Rebecca Diesing +4 more
doaj +1 more source
The surviving companions in type Ia supernova remnants [PDF]
L. Q. Chen, Xiangcun Meng, Zhanwen Han
openalex +1 more source
Supernova blast wave shock is a very important site of cosmic-ray acceleration. However, the detailed physical process of acceleration, in particular, nonlinear interplay between cosmic-ray streaming and magnetic field amplification, has not been studied
Tsuyoshi Inoue +2 more
doaj +1 more source
X-RAY EMISSION FROM STRONGLY ASYMMETRIC CIRCUMSTELLAR MATERIAL IN THE REMNANT OF KEPLER'S SUPERNOVA [PDF]
Mary T. Burkey +7 more
openalex +1 more source
MIXED-MORPHOLOGY SUPERNOVA REMNANTS IN X-RAYS: ISOTHERMAL PLASMA IN HB21 AND PROBABLE OXYGEN-RICH EJECTA IN CTB 1 [PDF]
Thomas G Pannuti +7 more
openalex +1 more source
Particle acceleration in supernova-remnant shocks [PDF]
S. P. Reynolds, S. P. Reynolds
openalex +1 more source
X-ray studies of supernova remnants: a different view of supernova explosions. [PDF]
Badenes C.
europepmc +1 more source
1051Ergs: The Evolution of Shell Supernova Remnants [PDF]
T. W. Jones +8 more
openalex +1 more source
Regions of Suppressed Diffusion around Supernova Remnants?
The recent discovery of the so-called TeV halos has attracted much attention. The morphology of the emission requires that the region is characterized by severe suppression of the diffusion coefficient. This finding raises many questions as to its origin:
Yiwei Bao, Pasquale Blasi, Yang Chen
doaj +1 more source
Dust in Supernovae and Supernova Remnants I: Formation Scenarios
A. Sarangi +3 more
semanticscholar +1 more source

