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The Manganese Star HD 1909

Published online by Cambridge University Press:  25 April 2016

W. Buscombe ,
C.R. Chambliss  and
Pamela M. Kennedy
Pamela M. Kennedy
Affiliation:
Mount Stromlo Observatory, Australian National University, Canberra
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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
Information
Publications of the Astronomical Society of Australia , Volume 1 , Issue 3 , February 1968 , pp. 84 - 85
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