On the source of the violet depression in carbon stars - A study of the Balmer decrement in carbon long-period variables

1987 ◽  
Vol 317 ◽  
pp. 819 ◽  
Author(s):  
Maria Antonietta Orlati
2000 ◽  
Vol 177 ◽  
pp. 367-375 ◽  
Author(s):  
T. Lloyd Evans

Spectroscopy and infrared photometry of carbon stars show three distinct forms of circumstellar matter. IRAS 12311-3509 probably has an edge-on disk and the spectrum is dominated by resonance emission from atoms and molecules in the vicinity. The long-period variables V Hya and R Lep are undergoing deep fadings, apparently caused by dust formation around the star, while variable emission from circumstellar gas is seen. The semiregular variable T Mus showed absorption bands from very cool material during an unusual episode in 1994.


Astrophysics ◽  
2019 ◽  
Vol 62 (2) ◽  
pp. 202-209
Author(s):  
N. Mauron ◽  
K. S. Gigoyan ◽  
K. K. Gigoyan ◽  
L. P. A. Maurin ◽  
T. R. Kendall

1994 ◽  
Vol 217 (1-2) ◽  
pp. 145-147
Author(s):  
P. Le Sidaner ◽  
T. Le Bertre

2003 ◽  
Vol 406 (1) ◽  
pp. 75-85 ◽  
Author(s):  
M. Rejkuba ◽  
D. Minniti ◽  
D. R. Silva

1998 ◽  
pp. 255-256
Author(s):  
F. Kerschbaum ◽  
B. Aringer ◽  
J. Hron ◽  
R. Loidl

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