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2006ApJ...652..362D - Astrophys. J., 652, 362-369 (2006/November-3)
A pulsational distance to ω Centauri based on near-infrared period-luminosity relations of RR Lyrae stars.
DEL PRINCIPE M., PIERSIMONI A.M., STORM J., CAPUTO F., BONO G., STETSON P.B., CASTELLANI M., BUONANNO R., CALAMIDA A., CORSI C.E., DALL'ORA M., FERRARO I., FREYHAMMER L.M., IANNICOLA G., MONELLI M., NONINO M., PULONE L. and RIPEPI V.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): Cosmology: Distance Scale - Galaxy: Globular Clusters: Individual: Name: ω Centauri - Stars: Evolution - Stars: Horizontal-Branch - Stars: Oscillations - Stars: Variables: Other
Simbad objects: 18
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