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A New SX Phe Star in the Globular Cluster M15
A new SX Phe star (labelled SXP1) found from CCD photometry is the first
to be discovered in the globular cluster M15. It is a blue straggler and is
located 102\arcsec.8 north and 285\arcsec.6 west of the center of M15
\citep{har96}. Mean magnitudes of SXP1 are = 18$\fm$671 and
= 18\fm445. The amplitude of variability of SXP1 is measured to be . From multiple-frequency analysis based on the Fourier
decomposition method, we detect two very closely separated pulsating
frequencies: the primary frequency at c/d for both - and
-bands, and the secondary frequency at c/d for the -band and
24.343 c/d for the -band. This star is the second among known SX Phe stars
found to pulsate with very closely separated frequencies ().
These frequencies may be explained by excitation of nonradial modes; however,
we have an incomplete understanding of this phenomenon in the case of SX Phe
stars with relatively high amplitudes. The metallicity-period and the
variability amplitude-period relations for SXP1 in M15 are found to be
consistent with those for SX Phe stars in other globular clusters.Comment: 15 pages with 6 figures, accepted by the Astronomical Journal
(scheduled May 2001
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