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The Manganese Star HD 1909

Published online by Cambridge University Press:  25 April 2016

Pamela M. Kennedy
Affiliation:
Mount Stromlo Observatory, Australian National University, Canberra

Extract

A coudé spectrogram of dispersion 150 µ/Å, exposed at the 74-inch reflector by D. S. Mathewson, reveals very many unusually sharp absorption lines due to ionized metals in the atmosphere of the B9 star HD 1909.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1968

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References

1 Westerlund, B.E., private communication, 1959.Google Scholar
2 Mihalas, D., Astrophys. J. Supp., 9, 321 (1965).Google Scholar
3 Buscombe, W., M.N.R.A.S., 126, 29 (1963).CrossRefGoogle Scholar
4 Auer, L. H. Mihalas, D., Aller, L.H., and Ross, J.E., Astrophys. J., 145, 153 (1966).CrossRefGoogle Scholar
5 Müller, Edith A., IAU Symposium, 26, 171 (1966).Google Scholar