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The Far UV Spectrum of the Binary System AX Mon*

Published online by Cambridge University Press:  23 September 2016

E. Danezis
E. Danezis*
Affiliation:
University of Athens, Laboratory of Astrophysics, Greece

Extract

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AX Mon is early indicated in the literature as a double system (Merrill 1952). Cowley (1964) noted that the system consists of a rapidly rotating B3 star and a somewhat fainter K giant.

We describe in this paper the main features of the far UV spectrum of HD 45910 observed with IUE at phase 0.5 (SWP 4762, LWR 4131). An analysis of this spectrum has been presented as part of a Ph.D. thesis (Danezis 1983). The far UV spectrum of AX Mon presents a large range of ionization stages going from CI, 01, NI, Mgl to SiIV, CIV, NV.

Type
IV. Models
Information
International Astronomical Union Colloquium , Volume 92: Physics of Be Stars , August 1987 , pp. 445 - 447
Copyright
Copyright © Cambridge University Press 1987

Footnotes

*

Read by V. Doazan

References

Cowley, A. P. 1964, Ap. J. 139, 817.Google Scholar
Danezis, E. 1983, Ph.D. Thesis, University of Athens 1983.Google Scholar
Merrill, P. W. 1952, Ap. J. 116, 498.CrossRefGoogle Scholar