On the use of Principal Component Analysis in analysing Cepheid light curves
Open Access
- 1 January 2002
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 329 (1) , 126-134
- https://doi.org/10.1046/j.1365-8711.2002.04948.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 6 references indexed in Scilit:
- The characteristics of second-overtone-mode Cepheids predicted by non-linear pulsation modelsMonthly Notices of the Royal Astronomical Society, 1997
- Long-Period Cepheids: Models and ObservationsThe Astrophysical Journal, 1995
- A dynamical systems approach to nonlinear stellar pulsationsAstrophysics and Space Science, 1993
- Observational studies of Cepheids. II - BVRI photometry of 112 CepheidsThe Astrophysical Journal Supplement Series, 1984
- The structural properties of Cepheid light curvesThe Astrophysical Journal, 1981
- Evidence Favoring Nonevolutionary Cepheid MassesThe Astrophysical Journal, 1976