The Valuable Long-period Cluster Cepheid KQ Scorpii and other Calibration Candidates

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Main Authors: Majaess, Daniel, Turner, David G., Minniti, Dante, Alonso-Garcia, Javier, Saito, Roberto K.
Format: Preprint
Published: 2024
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author Majaess, Daniel
Turner, David G.
Minniti, Dante
Alonso-Garcia, Javier
Saito, Roberto K.
author_facet Majaess, Daniel
Turner, David G.
Minniti, Dante
Alonso-Garcia, Javier
Saito, Roberto K.
contents The classical Cepheid KQ Sco is a valuable anchor for the distance scale because of its long pulsation period ($28^{\rm d}.7$) and evidence implying membership in the open cluster UBC 1558. Analyses tied to Gaia DR3 astrometry, photometry, spectroscopy, radial velocities, and 2MASS-VVV photometry indicate a common distance of $2.15\pm0.15$ kpc (\citealt{lin21} DR3 corrections applied). Additional cluster Cepheid candidates requiring follow-up are identified, and it's suggested that a team of international researchers could maintain a cluster Cepheid database to guide the broader community to cases where consensus exists.
format Preprint
id arxiv_https___arxiv_org_abs_2408_03371
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle The Valuable Long-period Cluster Cepheid KQ Scorpii and other Calibration Candidates
Majaess, Daniel
Turner, David G.
Minniti, Dante
Alonso-Garcia, Javier
Saito, Roberto K.
Solar and Stellar Astrophysics
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
The classical Cepheid KQ Sco is a valuable anchor for the distance scale because of its long pulsation period ($28^{\rm d}.7$) and evidence implying membership in the open cluster UBC 1558. Analyses tied to Gaia DR3 astrometry, photometry, spectroscopy, radial velocities, and 2MASS-VVV photometry indicate a common distance of $2.15\pm0.15$ kpc (\citealt{lin21} DR3 corrections applied). Additional cluster Cepheid candidates requiring follow-up are identified, and it's suggested that a team of international researchers could maintain a cluster Cepheid database to guide the broader community to cases where consensus exists.
title The Valuable Long-period Cluster Cepheid KQ Scorpii and other Calibration Candidates
topic Solar and Stellar Astrophysics
Cosmology and Nongalactic Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2408.03371