Hostname: page-component-8448b6f56d-mp689 Total loading time: 0 Render date: 2024-04-19T23:08:22.699Z Has data issue: false hasContentIssue false
  • English
  • Français

The Relation Between the Anomalous CN Strength, δ CN, and [FE/H] Abundances

Published online by Cambridge University Press:  04 August 2017

M. Fracassini ,
L. E. Pasinetti ,
L. Pastori  and
R. Pironi
M. Fracassini
Affiliation:
1Department of Physics, University of Milan
L. E. Pasinetti
Affiliation:
1Department of Physics, University of Milan
L. Pastori
Affiliation:
2Astronomical Observatory of Milano-Merate
R. Pironi
Affiliation:
1Department of Physics, University of Milan

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.

Following a previous study of stellar abundances (Pasinetti 1980), a relation has been derived between the DDO cyanogen-strength index and values of [Fe/H] reported in the catalog of Cayrel de Strobel, et al. (1980). From this relation we obtain [Fe/H] = 0.08 for the Hyades. This value is slightly lower than that given by Janes (1979), [Fe/H] = 0.13, and is in better agreement with other recent estimates of the Hyades metallicity (Cayrel de Strobel 1980). This improvement is due to the larger quantity of more precise spectroscopic data used in our correlation.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 111: Calibration of Fundamental Stellar Quantities , 1985 , pp. 427
Copyright
Copyright © Reidel 1985 

References

Cayrel de Strobel, G., Bentolila, C., Hauck, B. and Curchod, A. 1980, Astron. Astrophys. Suppl., 41, 405.Google Scholar
Cayrel de Strobel, G. 1980, in IAU Symposium No. 85, Star Clusters, ed. Hesser, J. E. (Reidel, Dordrecht), p. 91.Google Scholar
Janes, K. 1979, Astrophys. J. Suppl., 39, 135.Google Scholar
Pasinetti, L. E. 1980, in Cosmic Abundances of the Elements , ed. Hack, M., Mem. Soc. Astron. It., 51, 71.Google Scholar