Properties and Asteroseismological analysis of a new ZZ ceti discovered by TMTS
| Autor: | Jincheng Guo, Yanhui Chen, Xiaofeng Wang, Jie Lin, Gaobo Xi, Jun Mo, Alexei V Filippenko, Thomas Brink, Xiao-Yu Ma, Weikai Zong, Yong Yang, Jingkun Zhao, Xiangyun Zeng, Zhihao Chen, Ali Esamdin, Fangzhou Guo, Abdusamatjan Iskandar, Xiaojun Jiang, Wenxiong Li, Cheng Liu, Jianrong Shi, Xuan Song, Letian Wang, Danfeng Xiang, Shengyu Yan, Jicheng Zhang, Yonghui Yang |
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| Rok vydání: | 2023 |
| Předmět: | |
| Zdroj: | Monthly Notices of the Royal Astronomical Society. |
| ISSN: | 1365-2966 0035-8711 |
| Popis: | Tsinghua university-Ma Huateng Telescope for Survey (TMTS) aims to discover rapidly evolving transients by monitoring the northern sky. The TMTS catalog is cross-matched with the white dwarf (WD) catalog of Gaia EDR3, and light curves of more than a thousand WD candidates are obtained so far. Among them, the WD TMTS J23450729+5813146 (hereafter J2345) is one interesting common source. Based on the light curves from the TMTS and follow-up photometric observations, periods of 967.113 s, 973.734 s, 881.525 s, 843.458 s, 806.916 s and 678.273 s are identified. In addition, the TESS observations suggest a 3.39 h period but this can be attributed to the rotation of a comoving M dwarf located within 3". The spectroscopic observation indicates that this WD is DA type with Teff = 11778+/-617K,log g = 8.38+/-0.31,mass=0.84+/-0.20Msun and age=0.704+/-0.377 Gyrs. Asteroseismological analysis reveals a global best-fit solution of Teff =12110+/-10K and mass=0.760+/-0.005Msun,consistent with the spectral fitting results, and Oxygen and Carbon abundances in the core center are 0.73 and 0.27, respectively. The distance derived from the intrinsic luminosity given by asteroseismology is 93 parsec, which is in agreement with the distance of 98 parsec from Gaia DR3. Additionally, kinematic study shows that this WD is likely a thick disk star. The mass of its zero-age main-sequence mass is estimated to be 3.08 Msun and has a main-sequence plus cooling age of roughly 900 Myrs. 10 pages, 10 figures, accepted for publication in MNRAS |
| Databáze: | OpenAIRE |
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