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Origin of abundance inhomogeneity in globular clusters

✍ Scribed by K. Bekki; S. W. Campbell; J. C. Lattanzio; J. E. Norris

Book ID
110841784
Publisher
John Wiley and Sons
Year
2007
Tongue
English
Weight
433 KB
Volume
377
Category
Article
ISSN
0035-8711

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## Abstract Star‐to‐star variations in abundances of the light elements carbon, nitrogen, oxygen, and sodium have been observed in stars of all evolutionary phases in all Galactic globular clusters that have been thoroughly studied. The data available for studying this phenomenon, and the hypothese