Fabry-Perot measurements of the dynamics of globular cluster cores: M15 (NGC 7078)

1994 ◽  
Vol 107 ◽  
pp. 2067 ◽  
Author(s):  
K. Gebhardt ◽  
C. Pryor ◽  
T. B. Williams ◽  
James E. Hesser
1985 ◽  
pp. 89-92 ◽  
Author(s):  
Phyllis M. Lugger ◽  
Haldan Cohn ◽  
Jonathan E. Grindlay

2004 ◽  
Vol 348 (2) ◽  
pp. 679-686 ◽  
Author(s):  
Martin E. Beer ◽  
Melvyn B. Davies

1991 ◽  
Vol 381 ◽  
pp. 449 ◽  
Author(s):  
M. B. Davies ◽  
W. Benz ◽  
J. G. Hills

2007 ◽  
Vol 3 (S245) ◽  
pp. 189-190
Author(s):  
Mark Cropper ◽  
Dave Vande Putte

AbstractPrompted by the possibility that we have observed star formation triggered by globular cluster and dwarf spheroidal transits through galactic disks, we have examined kinematic evidence as to whether the superstar clusters in the Galactic bulge could have been formed from such transits. From their trajectores, we cannot exclude such a possibility. We note also that the high frequency of these transits may have generated rapid star formation at early times, and that remnant cluster cores may themselves nucleate further star formation.


1992 ◽  
Vol 401 ◽  
pp. 246 ◽  
Author(s):  
M. B. Davies ◽  
W. Benz ◽  
J. G. Hills

1985 ◽  
Vol 113 ◽  
pp. 73-76
Author(s):  
S. Djorgovski ◽  
H. Penner

We report the preliminary results of a surface photometry survey of globular cluster cores. Two new cores with post-collapse morphology have been found, and two possible candidates. The estimated fraction of clusters with this core morphology in the Galaxy is only a few percent. Most clusters do not show a morphology similar to the predictions of the central black hole models.


2009 ◽  
Vol 700 (2) ◽  
pp. 1233-1241 ◽  
Author(s):  
C. Y. Hui ◽  
K. S. Cheng ◽  
Ronald E. Taam
Keyword(s):  
X Ray ◽  

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