Results 31 to 40 of about 70 (69)

Helium Mixing in Globular Cluster Stars

, 1997
The observed abundance variations in globular cluster red giants indicate that these stars may be mixing helium from the hydrogen shell outward into the envelope, presumably as a result of internal rotation. We have investigated the implications of such helium mixing for both the red- giant-branch (RGB) and horizontal-branch (HB) phases by computing a ...
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Dynamics of Globular Star Clusters [PDF]

Europhysics News, 1989
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Helium in Globular Cluster Stars [PDF]

Nature, 1972
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On the Theory of Globular Star Clusters [PDF]

Monthly Notices of the Royal Astronomical Society, 1947
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Multicolour photometry of globular cluster stars

, 1977
The underlying theme of this thesis is the application of electronography to the study of stars in globular clusters through the use of both broad and intermediate-band photometric systems. Introductions to both the study of globular clusters and to the use of electronography are given in Chapter 1.
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Origin of the Globular Star Clusters

The Astrophysical Journal, 1968
P. J. E. Peebles, R. H. Dicke
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Accretion processes onto globular cluster stars

, 2000
Thoul, Anne, Jorissen, A., Goriely, S., Jehin, Emmanuel, Magain, Pierre, Noels-Grötsch, Arlette, Parmentier, Geneviève   +6 more
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Variable stars in galactic globular clusters

Astronomy & Astrophysics
Cruz Reyes, Mauricio, Anderson, Richard I., Johansson, Lucas, Netzel, Henryka, Medaric, Zoé   +4 more
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Abundance Anomalies in Globular Cluster Stars

EAS Publications Series, 2006
We present a summary of the extensive problems posed by the curious abundance correlations seen in stars in Galactic globular clusters. We discuss three scenarios, and conclude that only one seems to be consistent with the observations. Even this is still rather unsatisfying from many viewpoints.
J.C. Lattanzio, C.A. Tout
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Binary stars in globular clusters

1996
NOTE: Text or symbols not renderable in plain ASCII are indicated by [...]. Abstract is included in .pdf document. This thesis consists of several surveys to search for binary stars and to estimate the frequencies of binary populations in globular clusters.
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