Hostname: page-component-76fb5796d-vfjqv Total loading time: 0 Render date: 2024-04-26T23:57:28.442Z Has data issue: false hasContentIssue false

Population I Helium Burning Red Giants. Observations

Published online by Cambridge University Press:  25 April 2016

R. D. Cannon*
Affiliation:
Mount Stromlo and Siding Spring Observatories, Research School of Physical Sciences, Australian National University

Extract

The basic observational evidence for helium-burning red giants in open clusters has been given elsewhere, and I shall give here only a summary and then describe in more detail new results for one cluster, NGC 2477.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1971

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

1 Cannon, R. D., M.N.R.A.S., 150, 111 (1970).CrossRefGoogle Scholar
2 Burbidge, E. M. and Sandage, A. R., Ap. J., 128, 174 (1958).Google Scholar
3 Iben, I., Ap. J., 147, 624 (1967).Google Scholar
4 Iben, I., Ap. J., 147, 650 (1967).Google Scholar
5 Cannon, R. D. and Lloyd, C., M.N.R.A.S., 150, 279 (1970).Google Scholar
6 Faulkner, J., Ap. J., 144, 978 (1966)CrossRefGoogle Scholar
7 Faulkner, D. J., Proc. A.S.A., 2, 26 (1971).Google Scholar
8 Eggen, O. J. and Stoy, R. H., Roy. Obs. Bull., No. 24 (1961).Google Scholar