Carbon stars in the Large Magellanic Cloud - Photometry, spectroscopy, and evolutionary implications

1979 ◽  
Vol 230 ◽  
pp. 724 ◽  
Author(s):  
H. B. Richer ◽  
N. Olander ◽  
B. E. Westerlund
1978 ◽  
Vol 219 ◽  
pp. 452 ◽  
Author(s):  
H. B. Richer ◽  
B. E. Westerlund ◽  
N. Olander

2004 ◽  
Vol 355 (4) ◽  
pp. 1196-1206 ◽  
Author(s):  
D. H. Morgan ◽  
D. Hatzidimitriou ◽  
R. D. Cannon

2003 ◽  
Vol 341 (4) ◽  
pp. 1290-1298 ◽  
Author(s):  
D. Hatzidimitriou ◽  
D. H. Morgan ◽  
R. D. Cannon ◽  
B. F. W. Croke

Author(s):  
E. Marini ◽  
F. Dell'Agli ◽  
M. A. T. Groenewegen ◽  
D. A. García-Hernández ◽  
L. Mattsson ◽  
...  

2000 ◽  
Vol 540 (1) ◽  
pp. 211-216 ◽  
Author(s):  
David S. Graff ◽  
Andrew P. Gould ◽  
Nicholas B. Suntzeff ◽  
Robert A. Schommer ◽  
Eduardo Hardy

2018 ◽  
Vol 14 (S343) ◽  
pp. 504-505
Author(s):  
Sundar Srinivasan ◽  
I.-K. Chen ◽  
P. Scicluna ◽  
J. Cami ◽  
F. Kemper

AbstractIn order to investigate the effect of dust production on the molecular absorption, we model the dust continuum and the 7.5 and 13.7 μm acetylene absorption features in the Spitzer IRS spectra of 148 carbon stars in the Large Magellanic Cloud (LMC). Our preliminary investigation does not find a strong correlation between the dust-production rate and the column density of acetylene for the LMC sample. However, we will construct more models at high optical depths and probe a larger range of dust properties for more robust results.


Author(s):  
M. Matsuura ◽  
A.A Zijlstra ◽  
A.J Markwick ◽  
J.Th van Loon ◽  
I. Yamamura ◽  
...  

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