Problems and possibilities in fine-tuning of the Cepheid P-L relationship
arXiv:1201.1991 · doi:10.1007/s10509-012-0988-7
Abstract
Factors contributing to the scatter around the ridge-line period-luminosity relationship are listed, followed by a discussion how to eliminate the adverse effects of these factors (mode of pulsation, crossing number, temperature range, reddening, binarity, metallicity, non-linearity of the relationship, blending), in order to reduce the dispersion of the P-L relationship.
7 pages, 8 figures; accepted for publication in Astrophysics & Space Science
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- The influence of chemical composition on the properties of Cepheid stars. II-The iron content
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- A geometrical 1% distance to the short-period binary Cepheid V1334 Cygni
- Determination of the iron content of Cepheids from the shape of their light curves
- Discovery of the spectroscopic binary nature of six southern Cepheids
- Properties of the open cluster Tombaugh 1 from high resolution spectroscopy and uvbyCaH photometry
- Synthetic population of binary Cepheids. I. The effect of metallicity and initial parameter distribution on characteristics of Cepheids' companions
- Synthetic Population of Binary Cepheids. II. The effect of companion light on the extragalactic distance scale
- Discovery of the spectroscopic binary nature of the classical Cepheids FN Aql and V1344 Aql
- Non-evolutionary effects on period change in Magellanic Cepheids I. New binary systems revealed from Light Travel Time Effect
- Orbit determination for the binary Cepheid V1344 Aql
- Hunting for binary Cepheids using lucky imaging technique