The variable stars in the globular cluster Messier 28.

1949 ◽  
Vol 54 ◽  
pp. 193 ◽  
Author(s):  
Helen B. Sawyer
1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


2017 ◽  
Vol 468 (3) ◽  
pp. 2816-2821
Author(s):  
E. Martinazzi ◽  
S. O. Kepler ◽  
J. E. S. Costa

2009 ◽  
Author(s):  
Young-Beom Jeon ◽  
James M. Nemec ◽  
Alistair R. Walker ◽  
Joyce Ann Guzik ◽  
Paul A. Bradley

2013 ◽  
Vol 558 ◽  
pp. C1 ◽  
Author(s):  
J. Skottfelt ◽  
D. M. Bramich ◽  
R. Figuera Jaimes ◽  
U. G. Jørgensen ◽  
N. Kains ◽  
...  

2016 ◽  
Vol 587 ◽  
pp. C3
Author(s):  
R. Figuera Jaimes ◽  
A. Arellano Ferro ◽  
D. M. Bramich ◽  
S. Giridhar ◽  
K. Kuppuswamy

1989 ◽  
Vol 111 ◽  
pp. 285-285
Author(s):  
H.A. Smith ◽  
J.R. Kuhn ◽  
J. Curtis

AbstractBVR observations of the relatively metal-rich globular cluster NGC 6388 have been obtained with a CCD on the CTIO 0.9 m telescope. Eighteen possible short period variable stars have been discovered in or near the cluster. At least 10 of these are probable RR Lyrae members of NGC 6388. We confirm the finding of Hazen and Hesser that this cluster is one of the most metal-rich to contain a significant number of RR Lyraes. A program of CCD photometry of field and cluster variable stars has been initiated on the 0.6m telescope of the Michigan State University Observatory.


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