Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-06-15
Mon.Not.Roy.Astron.Soc.374:1421-1426,2007
Astronomy and Astrophysics
Astrophysics
6 pages, 9 figures. Accepted by MNRAS, major revision from previous version
Scientific paper
10.1111/j.1365-2966.2006.11247.x
[Fe/H] - phi_31 - log P relations are found for c-type RR Lyrae stars in globular clusters. The relations are analogous to that found by Jurcsik & Kovacs (1996) for field ab-type RR Lyrae stars, where a larger period correlates with lower metallicity values for similar values of the Fourier coefficient phi_31. The relations obtained here are used to determine the metallicity of field c-type RR Lyrae stars, those within omega Cen, the LMC and toward the galactic bulge. The results are found to compare favorably to metallicity values obtained elsewhere.
Morgan Siobahn M.
Wahl Jennifer N.
Wieckhorst Rachel M.
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