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Primary Period–Luminosity-Relation Calibrators in the Milky Way: Cepheids and RR Lyrae Physical basis, Calibration, and Applications

Published online by Cambridge University Press:  06 February 2024

M. A. T. Groenewegen Open the ORCID record for M. A. T. Groenewegen [Opens in a new window]
M. A. T. Groenewegen*
Affiliation:
Koninlijke Sterrenwacht van België, Ringlaan 3, 1180 Brussels, Belgium
*
martin.groenewegen@oma.be
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Abstract

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In this invited review I discuss the calibration and applications of the period–luminosity relation of classical Cepheid and RR Lyrae stars. After a brief introduction, starting with results from Hipparcos and discussing some post-Hipparcos era developments, I focus on recent results using Gaia Data Release 3 data. I present an overview of the most recent period–luminosity relations, a discussion and some new results on Cepheids in open clusters. I also discuss the effect of reddening and that the use of Wesenheit indices is actually an oversimplification to dealing with the problem of reddening.

Keywords

CepheidsRR LyraeDistance saleGalactic structure
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S376: At the crossroads of astrophysics and cosmology: Period–luminosity relations in the 2020s , December 2022 , pp. 128 - 149
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Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

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