Energy-spectroscopic studies of electron-capture processes by low-energy, highly stripped C, N, and O ions from He

1983 ◽  
Vol 28 (1) ◽  
pp. 127-134 ◽  
Author(s):  
K. Okuno ◽  
H. Tawara ◽  
T. Iwai ◽  
Y. Kaneko ◽  
M. Kimura ◽  
...  
1984 ◽  
Vol 29 (3) ◽  
pp. 1529-1532 ◽  
Author(s):  
H. Tawara ◽  
T. Iwai ◽  
Y. Kaneko ◽  
M. Kimura ◽  
N. Kobayashi ◽  
...  

1982 ◽  
Vol 26 (4) ◽  
pp. 1892-1906 ◽  
Author(s):  
R. A. Phaneuf ◽  
I. Alvarez ◽  
F. W. Meyer ◽  
D. H. Crandall
Keyword(s):  

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

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.


Radiocarbon ◽  
1992 ◽  
Vol 34 (3) ◽  
pp. 436-446 ◽  
Author(s):  
Walter Kutschera ◽  
Irshad Ahmad ◽  
Michael Paul

We have performed a new determination of the half-life of 41Ca by measuring the specific activity of an enriched Ca material with known 41Ca abundance. We measured the activity via the 3.3-keV X-rays emitted in the electron capture decay of 41Ca, and the 41Ca abundance was measured by low-energy mass spectrometry. The result, t1/2 = (1.01 ± 0.10) × 105 yr, agrees with the recent ‘geological’ half-life of Klein et al., (1991), t1/2 = (1.03 ± 0.07) × 105 yr, and with the corrected value of Mabuchi et al. (1974), t1/2 = (1.13 ± 0.12) × 105 yr. We recommend the weighted mean of these three measurements, t1/2 = (1.04 ± 0.05) × 105 yr, as the most probable half-life of 41Ca. We also discuss the situation of the radioisotopes, 32Si, 44Ti, 79Se and 126Sn, whose half-lives, though still uncertain, are potentially interesting for future AMS studies and other applications.


1992 ◽  
Vol 25 (13) ◽  
pp. 3009-3014 ◽  
Author(s):  
K Soejima ◽  
C J Latimer ◽  
K Okuno ◽  
N Kobayashi ◽  
Y Kaneko

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