Stellar encounters involving neutron stars in globular cluster cores

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

1996 ◽  
Vol 165 ◽  
pp. 389-400
Author(s):  
Helen M. Johnston ◽  
Frank Verbunt ◽  
Günther Hasinger ◽  
Wolfram Bunk

X-ray sources in globular clusters fall into two categories: the “bright” sources, with LX ∼ 1036-1038 erg s−1, and the “dim” sources, with LX ≲ 1034.5 erg s−1. The bright sources are clearly associated with accreting neutron stars in binary systems. The nature of the dim sources, however, remains in doubt. We review recent observations of globular-cluster X-ray sources with the ROSAT satellite. ROSAT detected bright sources in M31 globular clusters and greatly increased the number of dim sources known in galactic globular clusters. We discuss what these new observations have taught us about the distribution and nature of such sources, their spectral properties, and their underlying luminosity function.


Nature ◽  
1983 ◽  
Vol 301 (5901) ◽  
pp. 587-589 ◽  
Author(s):  
Piet Hut ◽  
Frank Verbunt

1994 ◽  
Vol 107 ◽  
pp. 2067 ◽  
Author(s):  
K. Gebhardt ◽  
C. Pryor ◽  
T. B. Williams ◽  
James E. Hesser

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.


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