Period--Luminosity Relations for Double-mode $δ$ Sct Stars
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arXiv
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2025
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| author | Jia, Qi Chen, Xiaodian Wang, Shu Deng, Licai Zhang, Jianxing Jiang, Qingquan |
| author_facet | Jia, Qi Chen, Xiaodian Wang, Shu Deng, Licai Zhang, Jianxing Jiang, Qingquan |
| contents | Previous studies of the Period--Luminosity relations (PLRs) of Delta Scuti ($δ$ Sct) stars have focused on those with a single pulsation mode. However, for $δ$ Sct stars with many different pulsation modes, classifying a single mode is difficult. In this study, an all-sky dataset is constructed using double-mode $δ$ Sct stars from ZTF and OGLE, and is used to determine F-mode and 1O-mode PLRs for eight single bands and six Wesenheit bands. In the $W1$ band, the PLR dispersion is about 0.171 mag and the total zero point error is 1\%. Our results show that to accurately classify the 1O modes of $δ$ Sct stars requires authentication based on multiple modes. Classification based on amplitude alone leads to impure 1O-mode $δ$ Sct stars and significant deviations in the PLRs. We compare the PLRs of the different sequences in the Petersen diagram and find that they are consistent after a strict criterion filtering, suggesting that their evolutionary state is similar. In addition, we find a weak period--metallicity relation for double-mode $δ$ Sct stars, unlike double-mode RR Lyrae stars. As distance tracers, large-amplitude F-mode $δ$ Sct and double-mode $δ$ Sct stars are the most suitable of the $δ$ Sct family. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2503_20557 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Period--Luminosity Relations for Double-mode $δ$ Sct Stars Jia, Qi Chen, Xiaodian Wang, Shu Deng, Licai Zhang, Jianxing Jiang, Qingquan Solar and Stellar Astrophysics Previous studies of the Period--Luminosity relations (PLRs) of Delta Scuti ($δ$ Sct) stars have focused on those with a single pulsation mode. However, for $δ$ Sct stars with many different pulsation modes, classifying a single mode is difficult. In this study, an all-sky dataset is constructed using double-mode $δ$ Sct stars from ZTF and OGLE, and is used to determine F-mode and 1O-mode PLRs for eight single bands and six Wesenheit bands. In the $W1$ band, the PLR dispersion is about 0.171 mag and the total zero point error is 1\%. Our results show that to accurately classify the 1O modes of $δ$ Sct stars requires authentication based on multiple modes. Classification based on amplitude alone leads to impure 1O-mode $δ$ Sct stars and significant deviations in the PLRs. We compare the PLRs of the different sequences in the Petersen diagram and find that they are consistent after a strict criterion filtering, suggesting that their evolutionary state is similar. In addition, we find a weak period--metallicity relation for double-mode $δ$ Sct stars, unlike double-mode RR Lyrae stars. As distance tracers, large-amplitude F-mode $δ$ Sct and double-mode $δ$ Sct stars are the most suitable of the $δ$ Sct family. |
| title | Period--Luminosity Relations for Double-mode $δ$ Sct Stars |
| topic | Solar and Stellar Astrophysics |
| url | https://arxiv.org/abs/2503.20557 |