SX Phe stars in globular clusters

DOI: 
Publication date: 
01/07/2000
Main author: 
Rodríguez E.
IAA authors: 
Rodríguez E.;López-González M.J.
Authors: 
Rodríguez E., López-González M.J.
Journal: 
Astronomy and Astrophysics
Publication type: 
Article
Volume: 
359
Pages: 
597-600
Number: 
Abstract: 
We present for the first time a catalogue of SX Phetype pulsating variables in globular clusters. In addition, SX Phe variables discovered in the Carina dwarf galaxy and other ones probably belonging to the Sagittarius dwarf galaxy are included. This catalogue is intended to be an up-dated list of all the SX Phe stars, in globular clusters and galaxies, known until now, covering information published up to January, 2000. In summary, 149 variables are presented in our list for SX Phe-type variables belonging to 18 globular clusters and 2 galaxies. Some relevant distributions are also shown. The analysis of metal abundances and mean periods shows that both parameters are correlated in the sense that the periods of the variables are longer as the metallicity of the stellar system is higher.
Database: 
WOK
SCOPUS
Keywords: 
Stars: fundamental parameters; Stars: oscillations; Stars: variables: general; Techniques: photometric