UV absorption investigation of ferromagnetically filled ultra-thick carbon onions, carriers of the 217.5 nm Interstellar Absorption Feature

2017 ◽  
Vol 122 (22) ◽  
pp. 224305 ◽  
Author(s):  
Filippo S. Boi ◽  
Xiaotian Zhang ◽  
Sameera Ivaturi ◽  
Qianyang Liu ◽  
Jiqiu Wen ◽  
...  
2003 ◽  
Vol 90 (15) ◽  
Author(s):  
Manish Chhowalla ◽  
H. Wang ◽  
N. Sano ◽  
K. B. K. Teo ◽  
S. B. Lee ◽  
...  

Nature ◽  
1980 ◽  
Vol 287 (5782) ◽  
pp. 518-519 ◽  
Author(s):  
D. T. Wickramasinghe ◽  
D. A. Allen

2011 ◽  
Vol 537 ◽  
pp. A27 ◽  
Author(s):  
M. Godard ◽  
T. R. Geballe ◽  
E. Dartois ◽  
G. M. Muñoz Caro

2017 ◽  
Vol 52 (14) ◽  
pp. 8362-8369 ◽  
Author(s):  
Jun Yan ◽  
Jian Zhang ◽  
Jinbo Tao ◽  
Danjing Hu ◽  
Qiujin Peng ◽  
...  

2019 ◽  
Vol 55 (2) ◽  
pp. 141-149
Author(s):  
D. Jack ◽  
K.-P. Schröder

We present a search and study of interstellar (IS) absorption features in the observed spectra of two Novae V339 Del and V5668 Sgr. We obtained high resolution spectra (R ≈ 20, 000) in the wavelength range between 3800 and 8800 Å of both novae with the TIGRE telescope. Common IS features of Na I and Ca II were identified in both novae, and the Ca II H and K features of Nova V339 Del show substructures, while a blueshifted absorption feature was found in the spectra of Nova V5668 Sgr. Absorption of K I was identified only in the spectra of Nova V5668 Sgr. The DIBs 6196, 6203, 6379, 6614 and 7562 were found in both novae, and in the spectra of Nova V5668 Sgr we could also identify the DIBs 5780, 5797 and 6660. We present the equivalent widths of all features and determined the column densities of Ca II, K I and hydrogen in the direction of Nova V5668 Sgr (log NCa II = 12.50, log NK I = 11.55, log NH = 18.5).


1997 ◽  
Vol 487 (2) ◽  
pp. 719-727 ◽  
Author(s):  
L. Henrard ◽  
Ph. Lambin ◽  
A. A. Lucas

Carbon ◽  
2004 ◽  
Vol 42 (1) ◽  
pp. 33-38 ◽  
Author(s):  
Yuki Kimura ◽  
Takeshi Sato ◽  
Chihiro Kaito

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