Shell type supernova remnants

1996 ◽  
Vol 75 (1-2) ◽  
Author(s):  
LO'C Drury
1967 ◽  
Vol 20 (3) ◽  
pp. 297 ◽  
Author(s):  
ER Hill

Radio evidence for two new supernova remnants in the Southern Milky Way is presented. Some new observations of the known supernova remnant, source 1439-62, and of the Rosette nebula, a shell source but not a supernova remnant, are also presented. The problem of finding model shells to fit the radio observations is considered and it is shown that the radio emission from 1439-62 is unlikely to originate in a shell with spherical symmetry.


2003 ◽  
Vol 29 (4) ◽  
pp. 641-664 ◽  
Author(s):  
A D Erlykin ◽  
A W Wolfendale

2001 ◽  
Vol 205 ◽  
pp. 398-399 ◽  
Author(s):  
Abdul I. Asvarov

It is shown that if the recently discovered hypernova events are intrinsically energetic spherically symmetric explosions of massive stars than they can leave after themselves very large diameter (up to 500 pc) nonthermal radio shells with spectral properties like ordinary shell type radio supernova remnants (SNRs). The properties of such shells are modeled and compared with the statistics of large diameter SNRs.


2008 ◽  
Vol 683 (2) ◽  
pp. L163-L166 ◽  
Author(s):  
Siming Liu ◽  
Zhong-Hui Fan ◽  
Christopher L. Fryer ◽  
Jian-Min Wang ◽  
Hui Li

2008 ◽  
Vol 484 (1) ◽  
pp. 267-273 ◽  
Author(s):  
J. Fang ◽  
L. Zhang ◽  
C. Y. Yang ◽  
G. F. Lin ◽  
A. M. Zheng

1996 ◽  
pp. 269-277 ◽  
Author(s):  
L. O’C Drury

2005 ◽  
Vol 444 (3) ◽  
pp. 893-893 ◽  
Author(s):  
H. J. Völk ◽  
E. G. Berezhko ◽  
L. T. Ksenofontov

2007 ◽  
Vol 309 (1-4) ◽  
pp. 379-384 ◽  
Author(s):  
M. Lemoine-Goumard ◽  
F. Aharonian ◽  
D. Berge ◽  
B. Degrange ◽  
D. Hauser ◽  
...  

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