No CrossRef data available.
Article contents
Carbon stars in the Small Magellanic Cloud: positions, finding charts and spectrophotometry
Published online by Cambridge University Press: 07 August 2017
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.
A survey for carbon stars in the Small Magellanic Cloud (SMC) has been carried out with the triplet camera at the prime focus of the ESO 3.6 m telescope using a Grism giving a dispersion of 2200 A/mm. 13 circular fields of 0.78 sq. degrees each, partially overlapping, cover the main body of the SMC (Rebeirot et al. 1987).
- Type
- Poster Papers
- Information
- Copyright
- Copyright © Kluwer
References
Azzopardi, M., Dumoulin, B., Quebatte, J. and Rebeirot, E. (1986), The Messenger
43, 12.Google Scholar
Azzopardi, M. and Rebeirot, E. (1991) IAU Symp. 148, in Haynes, R., Milne, D. (eds.), The Magellanic Clouds, Kluwer Academic Publishers, Dordrecht, pp. 71–76.Google Scholar
McCarthy, M.F. (1987) ESO conf. & Workshop Proc. No. 27, Azzopardi, M., Matteuci, F. (eds.) p. 203.Google Scholar
Rebeirot, E., Azzopardi, M., Breysacher, J. and Westerlund, B.E. (1987), ESO conf. & Workshop Proc. No. 27, Azzopardi, M., Matteuci, F. (eds.) p. 263.Google Scholar
Rebeirot, E., Azzopardi, M. and Westerlund, B.E. (1992) Astron. Astrophys. Suppl.
(in preparation).Google Scholar
Westerlund, B.E., Azzopardi, M. and Breysacher, J. (1986) Astron. Astrophys. Suppl.
65, 79.Google Scholar
You have
Access