Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-26T08:33:58.099Z Has data issue: false hasContentIssue false
  • English
  • Français

A Spectral Study of HD 50896

Published online by Cambridge University Press:  14 August 2015

V.S. Niemelä  and
R.H. Méndez
V.S. Niemelä
Affiliation:
Instituto de Astronomia y Fisica del Espacio, Buenos Aires, Argentina
R.H. Méndez
Affiliation:
Instituto de Astronomia y Fisica del Espacio, Buenos Aires, Argentina

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

ED 50896 (=EZ CMa) has long been known as a variable star. Recently, Firmani et al. (1980) derived a period of 3.763 days from spectral and photometric variations. This period was later confirmed by McLean (1980) and by Cherepashchuk (1981).

Type
SESSION 4 — OBSERVATIONS OF WOLF-RAYET BINARIES
Information
Symposium - International Astronomical Union , Volume 99: Wolf-Rayet Stars: Observations, Physics, Evolution , 1982 , pp. 295 - 298
Copyright
Copyright © Reidel 1982 

References

Cherepashchuk, A.M. 1981, M.N.R.A.S., 194, p.755.Google Scholar
Ebbets, D. 1979, P.A.S.P., 91, p. 804.Google Scholar
Firmani, C., Koenigsberger, G., Bisiacchi, G.F., Moffat, A.F.J. and Isserstedt, J. 1980, Ap. J., 239, p. 607.Google Scholar
McLean, I.S. 1980, Ap.J. (Letters), 236, p. L149.Google Scholar