Astronomy and Astrophysics – Astronomy
Scientific paper
May 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aas...21832209c&link_type=abstract
American Astronomical Society, AAS Meeting #218, #322.09; Bulletin of the American Astronomical Society, Vol. 43, 2011
Astronomy and Astrophysics
Astronomy
Scientific paper
The number of known SX Phoenicis (SX Phe) pulsators in Galactic globular clusters (GGCs) and the Local Group has more than doubled in recent years. Because all SX Phe in GGCs are likely blue stragglers, it has been suggested that their pulsational properties can constrain their evolutionary histories. We investigate the connection between SX Phe and blue stragglers via period-luminosity and color-magnitude diagrams. In particular, we verify distances to a large set of GGCs by fitting a carefully chosen set of nearby, unevolved subdwarfs to the cluster main sequences. We use these distances to analyze the pulsational properties of all known SX Phe, including SX Phe period-luminosity relations obtained using the SX Phe in these GGCs as calibrators, together with those in Local Group dwarf galaxies and their clusters. Finally, we discuss implications for blue straggler formation and evolution, and address both observational and theoretical avenues for further investigation.
Cohen Roger
Sarajedini Ata
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