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FeII in the UV Spectrum of Luminous Emission Line Stars

Published online by Cambridge University Press:  04 August 2017

G. Muratorio ,
M. Friedjung  and
R. Viotti
G. Muratorio
Affiliation:
Observatoire de Marseille, France
M. Friedjung
Affiliation:
Institut d'Astrophysique CNRS Paris, France
R. Viotti
Affiliation:
Instituto Astrofisica Spaziale CNR Frascati, Italy

Extract

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Following the excessive mass loss rates we derived in a previous analysis of the FeII emission and absorption lines of some luminous Magellanic Clouds stars, assuming the two components formed in the same region (Muratorio et al., 1984), we again analysed the FeII data using the same method (Muratorio, 1985), but taking into account the presence of high velocity winds detected in some stars (R66, R126) by the study of the high dispersion IUE spectra (Stahl et al., 1983; Zickgraf et al., 1985).

Type
Poster Papers 2
Information
Symposium - International Astronomical Union , Volume 116: Luminous Stars and Associations in Galaxies , 1986 , pp. 275 - 276
Copyright
Copyright © Reidel 1986 

References

Friedjung, M.: 1985, Astron. Astrophys. (in press) Google Scholar
Muratorio, G., Friedjung, M., Viotti, R.: 1984, Fourth European IUE conference Rome ESA SP 218 p. 309 Google Scholar
Muratorio, G.: 1985, Thèse de Doctorat d'Etat, Université Aix-Marseille I Google Scholar
Stahl, O., Wolf, B., Zickgraf, F. J., Bastian, V., De Groot, M. J. M., Leitherer, C.: 1983, Astron. Astrophys. 120, 287 Google Scholar
Zickgraf, F. J., Wolf, B., Stahl, O., Leitherer, C., Klare, G.: 1985, Astron. Astrophys. 143, 421 Google Scholar