A dipole band in 124Xe

1997 ◽  
Vol 359 (4) ◽  
pp. 347-348 ◽  
Author(s):  
G. Lo Bianco ◽  
Ch. Protochristov ◽  
G. Falconi ◽  
N. Blasi ◽  
D. Bazzacco ◽  
...  
Keyword(s):  
2012 ◽  
Vol 14 (5) ◽  
pp. 399-401
Author(s):  
Keyan Ma ◽  
Dong Yang ◽  
Jingbin Lu ◽  
Lielin Wang ◽  
Huidong Wang ◽  
...  
Keyword(s):  

1999 ◽  
Vol 59 (1) ◽  
pp. 71-81 ◽  
Author(s):  
J. Döring ◽  
D. Ulrich ◽  
G. D. Johns ◽  
M. A. Riley ◽  
S. L. Tabor

1998 ◽  
Vol 629 (3-4) ◽  
pp. 621-634 ◽  
Author(s):  
N. Nenoff ◽  
G. Baldsiefen ◽  
H. Hübel ◽  
A. Görgen ◽  
W. Korten ◽  
...  
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1997 ◽  
Vol 56 (3) ◽  
pp. 1338-1343 ◽  
Author(s):  
O. Vogel ◽  
A. Dewald ◽  
P. von Brentano ◽  
J. Gableske ◽  
R. Krücken ◽  
...  
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2019 ◽  
Vol 100 (4) ◽  
Author(s):  
C. G. Li ◽  
Q. B. Chen ◽  
S. Q. Zhang ◽  
C. Xu ◽  
H. Hua ◽  
...  
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1974 ◽  
Vol 52 (13) ◽  
pp. 1144-1151 ◽  
Author(s):  
A.R. W. McKellar

The 1–0, 2–0, 3–0, and 4–0 rotation–vibration bands of HD have been studied using a cooled multiple-traversal absorption cell and a grating spectrometer; intensities were measured for one electric quadrupole and 13 dipole transitions. There is particular interest in these intensities because HD has recently been detected on Jupiter by means of the 4–0 dipole band. Since the four bands were studied with the same gas samples and apparatus, possible errors in the measurement of their relative intensities were minimized. A rather large rotational dependence was found for the 1–0 band dipole transition moment. The present results are compared with theoretical intensity calculations, and it is concluded that there is good agreement for the quadrupole transition, but not for the dipole transitions.


2015 ◽  
Vol 92 (5) ◽  
Author(s):  
D. Hodge ◽  
D. M. Cullen ◽  
M. J. Taylor ◽  
M. G. Procter ◽  
P. Nieminen ◽  
...  
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