Tentative identification of the diffuse interstellar absorption bands and of a diffuse interstellar doublet line

1969 ◽  
Vol 3 (1) ◽  
pp. 102-108 ◽  
Author(s):  
Mogens Rudkj�bing
Nature ◽  
1968 ◽  
Vol 218 (5137) ◽  
pp. 153-153 ◽  
Author(s):  
W. W. DULEY

1973 ◽  
Vol 52 ◽  
pp. 327-333
Author(s):  
J. D. McCullough ◽  
G. R. Floyd ◽  
R. H. Prince ◽  
W. W. Duley

The possibility that many different diffuse interstellar absorption features may be produced by the same type of absorbing atom in different hydrocarbon matrices on interstellar grains has been examined experimentally. The present study shows that absorption bands due to Na atoms in various hydrocarbon matrices can occur within the wavelength range 5400–5800 Å. A study of the molecules generated from the radiation-induced polymerization of C2H2 at 55 K is also reported. It is shown that C6H6 is an abundant product of this polymerization and may therefore be an important constituent of interstellar grains.


Nature ◽  
1994 ◽  
Vol 369 (6478) ◽  
pp. 296-298 ◽  
Author(s):  
B. H. Foing ◽  
P. Ehrenfreund

2009 ◽  
Vol 52 (4) ◽  
pp. 489-501 ◽  
Author(s):  
FuYuan Xiang ◽  
ShunLin Liang ◽  
AiGen Li

Nature ◽  
1981 ◽  
Vol 294 (5838) ◽  
pp. 239-240 ◽  
Author(s):  
D. A. Allen ◽  
D. T. Wickramasinghe

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