Eppur binaria non è esclusa: Pulsations in CZ Tuc appear to be tidally excited by its veiled companion
Abstract
Long secondary periods (LSPs), observed in about one-third of pulsating red giants, remain unexplained despite decades of study, with binarity and non-radial oscillations as the leading competing hypotheses. If LSP variables are indeed interacting, eccentric binary systems consisting of a red giant and a substellar object, tidally excited oscillations (TEOs) would be expected to appear in a fraction of them. Therefore, detection of TEOs offers an independent test of the binary scenario that has not previously been applied to LSP stars. Using a combined, approximately 80-year light curve assembled from Digital Access to a Sky Century @ Harvard (DASCH), Hipparcos, and All Sky Automatic Survey (ASAS) photometry, we find that CZ Tucanae (CZ Tuc) exhibits a pulsation period of 55.4734±0.0074 days along with its LSP of 443.62±0.12 days, with a ratio of 7.9970±0.0024 - consistent with a TEO. Theoretical models show the observed amplitude of the candidate TEO could be produced after adopting the estimated fundamental parameters of CZ Tuc. Our findings identify CZ Tuc as the first candidate LSP star with a TEO, providing independent evidence for binarity among at least a subset of these enigmatic variables.
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BibTeX
@misc{kolaczekszymanski2026eppur,
title = {{Eppur binaria non è esclusa: Pulsations in CZ Tuc appear to be tidally excited by its veiled companion}},
author = {Piotr A. Kołaczek-Szymański and Patryk Iwanek and Jim Fuller and Dorota M. Skowron and Grzegorz Pojmański and Igor Soszyński},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.00471},
eprint = {2610.00471},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.00471},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Eppur binaria non è esclusa: Pulsations in CZ Tuc appear to be tidally excited by its veiled companion
AU - Piotr A. Kołaczek-Szymański
AU - Patryk Iwanek
AU - Jim Fuller
AU - Dorota M. Skowron
AU - Grzegorz Pojmański
AU - Igor Soszyński
PY - 2026
DA - 2026/10/01
PB - arXiv
DO - 10.48550/arxiv.2610.00471
UR - https://arxiv.org/abs/2610.00471
AB - Long secondary periods (LSPs), observed in about one-third of pulsating red giants, remain unexplained despite decades of study, with binarity and non-radial oscillations as the leading competing hypotheses. If LSP variables are indeed interacting, eccentric binary systems consisting of a red giant and a substellar object, tidally excited oscillations (TEOs) would be expected to appear in a fraction of them. Therefore, detection of TEOs offers an independent test of the binary scenario that has not previously been applied to LSP stars. Using a combined, approximately 80-year light curve assembled from Digital Access to a Sky Century @ Harvard (DASCH), Hipparcos, and All Sky Automatic Survey (ASAS) photometry, we find that CZ Tucanae (CZ Tuc) exhibits a pulsation period of 55.4734±0.0074 days along with its LSP of 443.62±0.12 days, with a ratio of 7.9970±0.0024 - consistent with a TEO. Theoretical models show the observed amplitude of the candidate TEO could be produced after adopting the estimated fundamental parameters of CZ Tuc. Our findings identify CZ Tuc as the first candidate LSP star with a TEO, providing independent evidence for binarity among at least a subset of these enigmatic variables.
ER -