EPR spectroscopic study of the reaction of ground-state aluminium atoms with acyclic alcohols in a rotating cryostat

2001 ◽  
Vol 3 (5) ◽  
pp. 750-759 ◽  
Author(s):  
Helen A. Joly ◽  
James A. Howard ◽  
Gustavo A. Arteca
1988 ◽  
Vol 92 (10) ◽  
pp. 2745-2750 ◽  
Author(s):  
J. H. B. Chenier ◽  
C. A. Hampson ◽  
J. A. Howard ◽  
B. Mile

1993 ◽  
Vol 287 ◽  
pp. 107-110
Author(s):  
P. Fernández-Serra ◽  
Y.G. Smeyers ◽  
A. Galano ◽  
G.Delgado Barrio

2006 ◽  
Vol 74 (11) ◽  
Author(s):  
K. Kuepper ◽  
R. Klingeler ◽  
P. Reutler ◽  
B. Büchner ◽  
M. Neumann

1995 ◽  
Vol 91 (5) ◽  
pp. 799 ◽  
Author(s):  
J. A. Howard ◽  
C. McCague ◽  
R. Sutcliffe ◽  
J. S. Tse ◽  
H. A. Joly

2008 ◽  
Vol 77 (20) ◽  
Author(s):  
Masazumi Fujiwara ◽  
Kensei Yamauchi ◽  
Mitsuru Sugisaki ◽  
Andrew Gall ◽  
Bruno Robert ◽  
...  

2012 ◽  
Vol 5 (3) ◽  
pp. 698-715 ◽  
Author(s):  
Chen Song ◽  
Lars-Oliver Essen ◽  
Wolfgang Gärtner ◽  
Jon Hughes ◽  
Jörg Matysik

2004 ◽  
Vol 194 ◽  
pp. 237-237
Author(s):  
S. Kafka ◽  
C. Tappert ◽  
R. K. Honeycutt ◽  
A. Bianchini

A time-resolved optical spectroscopic study of the long-period (P=10.08h) old nova Q Cyg has revealed persistent yet erratic absorption features indicating the presence of a wind, while the system was rising to one of its stunded outbursts. Data taken with the WIYN 3.5m telescope show P Cygni profiles in the He I triplet lines at 5876Å and 7065Å, which are absent in the He I singlet emission line at 6678Å, despite the fact that the relevant energy levels of those three lines are at very similar excitation levels. The Hα line often has a red ward emission tail, characteristic of a receding outflow, and it possess a blueward absorption profile during only one wind event. Kafka et al. (2003) argued that this behavior is due to the strongly metastable 2 3S effective ground state of the He I triplets, which becomes over-populated in conditions of low density and a dilute radiation field, over-populating in turn the 23P common lower level of He I 5876Å and 7065Å, leading to absorption from a low density wind. Therefore, the triplet/singlet lines trace two different parts of the system: the wind and the disk respectively.


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