Henrietta Leavitt's classical Cepheid relation
Abstract
The Leavitt & Pickering (1912) mean period-magnitude relation for SMC Cepheids exhibits correlated residuals relative to modern Gaia BG and Johnson V photometry (rδV/δL12≈0.76). Therefore dispersion inherent to Leavitt's photographic photometry relation is not solely random scatter (σL12,BG,V=0.22±0.03,0.25±0.04,0.20±0m.03), and is potentially consistent with the partial encoding of combined effects from the elongated SMC, classical Cepheid instability strip, differential reddening, etc. OGLE data indicate that ≳870 SMC variables identified by Leavitt (1908, Table 2) are classical Cepheids (≳ 90 %), and the preliminary unphased Table 2 photometry likewise features correlated residuals relative to contemporary observations (rδBG/δL08−T2≈0.54). Table 6 data in Leavitt (1908, n=16) define a highly linear Leavitt law over an extensive baseline (r≈−0.98), but constitute a smaller sample than the later 1912 work (n=25).
Related
- Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: X First spectroscopic characterization of Galactic Type II Cepheids and calibration of the Period-Wesenheit-Metallicity relations
- Multi-chromatic observations of classical Cepheids using the CHARA Array interferometer: Surface brightness-colour relation, projection factor, and limb-darkening
- Convection in the interior of Cepheid variable stars
- A Cepheid-based Distance to the Type 1 Seyfert NGC 3783
- Age Discrepancy in Three Galactic Cepheid Binaries
BibTeX
@misc{majaess2026henrietta,
title = {{Henrietta Leavitt's classical Cepheid relation}},
author = {Daniel Majaess},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.17415},
eprint = {2610.17415},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.17415},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Henrietta Leavitt's classical Cepheid relation
AU - Daniel Majaess
PY - 2026
DA - 2026/10/12
PB - arXiv
DO - 10.48550/arxiv.2610.17415
UR - https://arxiv.org/abs/2610.17415
AB - The Leavitt & Pickering (1912) mean period-magnitude relation for SMC Cepheids exhibits correlated residuals relative to modern Gaia B_G and Johnson V photometry (r_δV/δL12≈0.76). Therefore dispersion inherent to Leavitt's photographic photometry relation is not solely random scatter (σ_L12,B_G,V=0.22±0.03,0.25±0.04,0.20±0^m.03), and is potentially consistent with the partial encoding of combined effects from the elongated SMC, classical Cepheid instability strip, differential reddening, etc. OGLE data indicate that ≳870 SMC variables identified by Leavitt (1908, Table 2) are classical Cepheids (≳ 90 %), and the preliminary unphased Table 2 photometry likewise features correlated residuals relative to contemporary observations (r_δB_G/δL08−T2≈0.54). Table 6 data in Leavitt (1908, n=16) define a highly linear Leavitt law over an extensive baseline (r≈−0.98), but constitute a smaller sample than the later 1912 work (n=25).
ER -