Empirical P-L-C relation for δ scuti stars

DOI: 
10.1007/BF00640715
Publication date: 
01/07/1990
Main author: 
López de Coca P.
IAA authors: 
López de Coca P.;Rolland A.;Garrido R.;Rodriguez E.
Authors: 
López de Coca P., Rolland A., Garrido R., Rodriguez E.
Journal: 
Astrophysics and Space Science
Publication type: 
Article
Volume: 
169
Pages: 
211-213
Number: 
Abstract: 
Empirical period-luminosity-colour (P-L-C) relations are obtained for the four lowest modes corresponding to radial pulsations. Agreement with predicted values indicates that, in general, both Strömgren photometric calibration and pulsation theory work well for these stars. © 1990 Kluwer Academic Publishers.
Database: 
SCOPUS
ADS
URL: 
https://ui.adsabs.harvard.edu/#abs/1990Ap&SS.169..211L/abstract
ADS Bibcode: 
1990Ap&SS.169..211L
Keywords: