The Velocity Structure of Large Magellanic Cloud Carbon Stars: Young Disk, Old Disk, and Perhaps a Separate Population

2000 ◽  
Vol 540 (1) ◽  
pp. 211-216 ◽  
Author(s):  
David S. Graff ◽  
Andrew P. Gould ◽  
Nicholas B. Suntzeff ◽  
Robert A. Schommer ◽  
Eduardo Hardy
Keyword(s):  
Velocity Structure ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Carbon Stars ◽  
Separate Population

Three luminous carbon stars in the Large Magellanic Cloud

1978 ◽  
Vol 219 ◽  
pp. 452 ◽  
Author(s):  
H. B. Richer ◽  
B. E. Westerlund ◽  
N. Olander
Keyword(s):  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Carbon Stars

Merrill-Sanford bands in Large Magellanic Cloud carbon stars

2004 ◽  
Vol 355 (4) ◽  
pp. 1196-1206 ◽  
Author(s):  
D. H. Morgan ◽  
D. Hatzidimitriou ◽  
R. D. Cannon
Keyword(s):  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Carbon Stars

scholarly journals Lithium in Large Magellanic Cloud carbon stars

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

scholarly journals Understanding the evolution and dust formation of carbon stars in the Large Magellanic Cloud via the JWST

2021 ◽  
Author(s):  
E. Marini ◽  
F. Dell'Agli ◽  
M. A. T. Groenewegen ◽  
D. A. García-Hernández ◽  
L. Mattsson ◽  
...  
Keyword(s):  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Dust Formation ◽  
Carbon Stars

Modelling gas and dust around carbon stars in the Large Magellanic Cloud

2018 ◽  
Vol 14 (S343) ◽  
pp. 504-505
Author(s):  
Sundar Srinivasan ◽  
I.-K. Chen ◽  
P. Scicluna ◽  
J. Cami ◽  
F. Kemper
Keyword(s):  
Production Rate ◽  
Strong Correlation ◽  
Column Density ◽  
Preliminary Investigation ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Carbon Stars ◽  
Molecular Absorption ◽  
Dust Production ◽  
Absorption Features

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.

Three Micron Spectra of Carbon Stars in the Large Magellanic Cloud

2003 ◽  
pp. 259-262
Author(s):  
M. Matsuura ◽  
A.A Zijlstra ◽  
A.J Markwick ◽  
J.Th van Loon ◽  
I. Yamamura ◽  
...  
Keyword(s):  
Large Magellanic Cloud ◽  
Magellanic Cloud ◽  
Carbon Stars
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