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Infra-red Observations of Globular Cluster Giants
Published online by Cambridge University Press: 25 April 2016
Extract
This paper presents a progress report on a programme of infra-red photoelectric photometry of the red giant sequences in some southern globular clusters. As measured in B and V these sequences are known to differ from cluster to cluster, at least one contributing factor being differential line-blanketing arising from variations in metal abundance. Observations in R and I should be substantially free of blanketing, and so enable us to eliminate this factor, clarifying the situation and making possible a more accurate transformation of the observations to the Mbol, log Tett plane. The difficulty of making this transformation has been a major obstacle in comparing observations and theory for cluster giants.
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- Information
- Publications of the Astronomical Society of Australia , Volume 1 , Issue 3 , February 1968 , pp. 83 - 84
- Copyright
- Copyright © Astronomical Society of Australia 1968