Abstract
Nemec: The recent finding by Nemec, Nemec and Norris (1986 Astron. J. 92), and others, that double-mode RR Lyrae stars are not found in the highly flattened globular cluster ω Cen, despite the apparent similarity of the primary periods of these stars to the primary (first overtone) periods of the double-mode RR Lyrae stars in M 15, seems to us might also be caused by star-to-star angular momentum differences.
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© 1988 International Astronomical Union
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Grindlay, J.E., Davis Philip, A.G. (1988). Discussion. In: Grindlay, J.E., Davis Philip, A.G. (eds) The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies. International Astronomical Union / Union Astronomique Internationale, vol 126. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-1104-9_14
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DOI: https://doi.org/10.1007/978-94-015-1104-9_14
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