[Fe/H] - φ 31 - Period relation for c-type RR Lyrae Variables

Details [Fe/H] - φ 31 - Period relation for c-type RR Lyrae Variables [Fe/H] - φ 31 - Period relation for c-type RR Lyrae Variables

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...206.4103w&link_type=abstract

American Astronomical Society Meeting 206, #41.03; Bulletin of the American Astronomical Society, Vol. 37, p.495

Astronomy and Astrophysics

Astronomy

Scientific paper

A [Fe/H] - φ 31 - Period relation is found for c-type RR Lyra stars in globular clusters. The relation is analogous to that found by Jurcsik & Kovacs (1996) for field ab-type RR Lyra stars, where a larger period correlates with lower metallicity values for similar values of the Fourier coefficient φ 31. The metallicity of field c-type RR Lyra stars and those within ω Cen are also examined using the new relation and these results are also presented.

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