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Chemical Content of Nine F-Supergiants from Different Regions of the LMC

Published online by Cambridge University Press:  07 August 2017

V. Hill
V. Hill*
Affiliation:
DASGAL/URA 335 du C.N.R.S. - Observatoire de Paris-Meudon, F-92195, Meudon Cedex - E-mail: [email protected]

Extract

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In order to extend the available abundance information in the Magellanic Clouds, and particularly the elemental ratios, we have undertaken a homogenous sudy of supergiants stars in both Clouds using high resolution spectroscopy. We compare the abundance ratios obtained for nine LMC F-supergiants (Hill et al., 1994) with those for three SMC similar stars (Spite et al., 1989).

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 164: Stellar Populations , 1995 , pp. 416
Copyright
Copyright © Kluwer 1995 

References

Hill, V., Andrievsky, S. and Spite, M. (1994), A&A, in press Google Scholar
Spite, M., Barbuy, B. and Spite, F. (1989), A&A, Vol. 222, pp. 35–40 Google Scholar