The MACHO Project LMC Variable Star Inventory. VII. The Discovery of RV Tauri Stars and New Type II Cepheids in the Large Magellanic Cloud

1998 ◽  
Vol 115 (5) ◽  
pp. 1921-1933 ◽  
Author(s):  
C. Alcock ◽  
R. A. Allsman ◽  
D. R. Alves ◽  
T. S. Axelrod ◽  
A. Becker ◽  
...  
2003 ◽  
Vol 598 (1) ◽  
pp. 597-609 ◽  
Author(s):  
C. Alcock ◽  
D. R. Alves ◽  
A. Becker ◽  
D. Bennett ◽  
K. H. Cook ◽  
...  

2002 ◽  
Vol 573 (1) ◽  
pp. 338-350 ◽  
Author(s):  
C. Alcock ◽  
R. A. Allsman ◽  
D. R. Alves ◽  
A. C. Becker ◽  
D. P. Bennett ◽  
...  

1996 ◽  
Vol 470 ◽  
pp. 583 ◽  
Author(s):  
C. Alcock ◽  
R. A. Allsman ◽  
D. R. Alves ◽  
T. S. Axelrod ◽  
A. Becker ◽  
...  

1963 ◽  
Vol 68 ◽  
pp. 281 ◽  
Author(s):  
P. W. Hodge ◽  
F. W. Wright

2017 ◽  
Vol 153 (4) ◽  
pp. 154 ◽  
Author(s):  
Anupam Bhardwaj ◽  
Lucas M. Macri ◽  
Marina Rejkuba ◽  
Shashi M. Kanbur ◽  
Chow-Choong Ngeow ◽  
...  

1991 ◽  
Vol 148 ◽  
pp. 384-385
Author(s):  
Douglas L. Welch ◽  
Patrick Côté ◽  
Mario Mateo ◽  
Barry F. Madore

We report the results of an extensive photometric and radial velocity study of the variable stars in the Large Magellanic Cloud (LMC) cluster NGC 1866. We find:


2014 ◽  
Vol 446 (3) ◽  
pp. 3034-3061 ◽  
Author(s):  
V. Ripepi ◽  
M. I. Moretti ◽  
M. Marconi ◽  
G. Clementini ◽  
M.-R. L. Cioni ◽  
...  

2010 ◽  
Vol 6 (S272) ◽  
pp. 541-542 ◽  
Author(s):  
Thomas Rivinius ◽  
Ronald E. Mennickent ◽  
Zbigniew Kołaczkowski

AbstractBI 108 is a luminous variable star in the Large Magellanic Cloud classified B1 II. The variability consists of two resonant periods (3:2), of which only one is orbital, however. We discuss possible mechanisms responsible for the second period and its resonant locking.


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