Low-energy resonance states upon electron capture by five-membered heterocycles and cyclopentadiene

Author(s):  
M. V. Muftakhov ◽  
V. A. Mazunov ◽  
V. I. Khvostenko

1990 ◽  
Vol 26 (2) ◽  
pp. 240-241
Author(s):  
M. V. Muftakhov ◽  
V. A. Mazunov ◽  
V. I. Khvostenko


1989 ◽  
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2001 ◽  
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1982 ◽  
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pp. 1892-1906 ◽  
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I. Alvarez ◽  
F. W. Meyer ◽  
D. H. Crandall
Keyword(s):  


1983 ◽  
Vol 28 (1) ◽  
pp. 127-134 ◽  
Author(s):  
K. Okuno ◽  
H. Tawara ◽  
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Y. Kaneko ◽  
M. Kimura ◽  
...  


1965 ◽  
Vol 38 (2) ◽  
pp. 872-882 ◽  
Author(s):  
H. Burkhardt ◽  
G. P. McCauley


2020 ◽  
Vol 37 (2) ◽  
pp. 023401 ◽  
Author(s):  
Kun Wang ◽  
Xiao-Xia Wang ◽  
Yi-Zhi Qu ◽  
Chun-Hua Liu ◽  
Ling Liu ◽  
...  


2019 ◽  
Vol 795 ◽  
pp. 122-128 ◽  
Author(s):  
A. Boeltzig ◽  
A. Best ◽  
F.R. Pantaleo ◽  
G. Imbriani ◽  
M. Junker ◽  
...  


2019 ◽  
Vol 52 (7) ◽  
pp. 075202
Author(s):  
K Wang ◽  
Y Z Qu ◽  
C H Liu ◽  
L Liu ◽  
Y Wu ◽  
...  


2020 ◽  
Vol 7 (7) ◽  
pp. 200467
Author(s):  
Morgan Fraser

It is 30 years since the characteristic signatures of interaction with circumstellar material (CSM) were first observed in a core-collapse supernova. Since then, CSM interaction has been observed and inferred across a range of transients, from the low-energy explosions of low-mass stars as likely electron-capture supernovae, through to the brightest superluminous supernovae. In this review, I present a brief overview of some of the interacting supernovae and transients that have been observed to date, and attempt to classify and group them together in a phenomenological framework.



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