Results 151 to 160 of about 201,431 (246)

Nonthermal Signatures of Radiative Supernova Remnants

open access: yesThe Astrophysical Journal
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]

open access: bronze, 2017
L. Q. Chen, Xiangcun Meng, Zhanwen Han
openalex   +1 more source

Bell Instability–mediated Diffusive Shock Acceleration at Supernova Blast Wave Shock Propagating in the Interstellar Medium

open access: yesThe Astrophysical Journal
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]

open access: bronze, 2013
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]

open access: bronze, 2010
Thomas G Pannuti   +7 more
openalex   +1 more source

1051Ergs: The Evolution of Shell Supernova Remnants [PDF]

open access: hybrid, 1998
T. W. Jones   +8 more
openalex   +1 more source

Regions of Suppressed Diffusion around Supernova Remnants?

open access: yesThe Astrophysical Journal
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

open access: yesSupernovae, 2018
A. Sarangi   +3 more
semanticscholar   +1 more source

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