期刊
ASTROPHYSICAL JOURNAL
卷 685, 期 2, 页码 947-957出版社
UNIV CHICAGO PRESS
DOI: 10.1086/591241
关键词
blue stragglers; delta Scuti; galaxies : distances and redshifts; galaxies : individual (Fornax); stars : variables : other; techniques : photometric
资金
- PRIN INAF [39/2005]
We have carried out an intensive survey of the northern region of the Fornax dwarf spheroidal galaxy with the aim of detecting the galaxy's short-period pulsating stars (P < 0.25 days). Observations collected over three consecutive nights with the Wide Field Imager of the 2.2 m MPI telescope at ESO allowed us to detect 85 high-amplitude (0.20-1.00 mag in B light) variable stars with periods in the range from 0.046 to 0.126 days, similar to SX Phoenicis stars in Galactic metal-poor stellar populations. The plots of the observed periods vs. the B and V magnitudes show a dispersion largely exceeding the observational errors. To disentangle the matter, we separated the first-overtone from the fundamental-mode pulsators and tentatively identified a group of subluminous variables, about 0.35 mag fainter than the others. Their nature as either metal-poor intermediate-age stars or stars formed by the merging of close binary systems is discussed. The rich sample of the Fornax variables also led us to reconstruct the period-luminosity relation for short-period pulsating stars. An excellent linear fit, M-V - -1.83(+/- 0.08) - 3.65(+/- 0.07) log P-F, was obtained using 153 delta Scuti and SX Phoenicis stars in a number of different stellar systems.
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