Knowledge Management System of Institute of Theoretical Physics, CAS
| Xue, HF; Fu, JN; Fox-Machado, L; Shi, JR; Zhou, YT; Zhang, JB; Michel, R; Yan, HL; Niu, JS; Zong, WK; Su, J7; Castro, A; Ayala-Loera, C; Altamirano-Devora, L | |
| Asteroseismology of the Double-mode High-amplitude delta Scuti Star VX Hydrae | |
| Source Publication | ASTROPHYSICAL JOURNAL
 |
| Language | 英语 |
| Keyword | EQUATION-OF-STATE STELLAR EVOLUTION PERIOD CHANGES PULSATION OPACITIES |
| Abstract | Bi-site time-series photometric and high-resolution spectroscopic observations were made for the double-mode high-amplitude delta Scuti star VX Hya. The fundamental frequency f(0) = 4.4763 c days(-1), the first overtone f(1) = 5.7897 c days(-1), and 23 harmonics and linear combinations of f(0) and f(1) are detected by pulsation analysis. From the spectroscopic data, we get [Fe/H] = -0.2 +/- 0.1 dex. The period change rate of the fundamental mode is obtained by using the Fourier-phase diagram method, which gives the value of (1/P-0)(dP(0)/dt) = (1.81 +/- 0.09) x 10(-7) yr(-1). With these results from the observations, we perform theoretical explorations with the stellar evolution code MESA, and constrain the models by fitting f(0), f(1), and (1/P-0)(dP(0)/dt) within 3 sigma deviations. The results show that the period change of VX Hya could be ascribed to the evolutionary effect. The stellar parameters of VX Hya could be derived as: the mass 2.385 +/- 0.025M(circle dot), the luminosity log(L/L-circle dot) = 1.93 +/- 0.02, and the age (4.43 +/- 0.13) x 10(8) years. VX Hya is found to locate at the post-main-sequence stage with a helium core and a hydrogen-burning shell on the H-R diagram. |
| 2018 | |
| ISSN | 0004-637X |
| Volume | 861Issue:2Pages:96 |
| Subject Area | Astronomy & Astrophysics |
| MOST Discipline Catalogue | Astronomy & Astrophysics |
| DOI | 10.3847/1538-4357/aac9c5 |
| Indexed By | SCIE |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.itp.ac.cn/handle/311006/22867 |
| Collection | SCI期刊论文 |
| Affiliation | 1.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China 2.Fox-Machado, L.; Michel, R.; Castro, A.; Ayala-Loera, C.; Altamirano-Devora, L.] Univ Nacl Autonoma Mexico, Observ Astron Nacl, Inst Astron, Ap P 877, Ensenada 22860, Baja California, Mexico 3.Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, Beijing 100012, Peoples R China 4.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 5.Shanxi Univ, Inst Theoret Phys, Taiyuan 030006, Peoples R China 6.Chinese Acad Sci, Inst Theoret Phys, Key Lab Theoret Phys, Beijing 100190, Peoples R China 7.Univ Chinese Acad Sci, Sch Phys Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China 8.Chinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China 9.Castro, A.] Univ Southampton, Phys & Astron, Southampton SO17 1BJ, Hants, England |
| Recommended Citation GB/T 7714 | Xue, HF,Fu, JN,Fox-Machado, L,et al. Asteroseismology of the Double-mode High-amplitude delta Scuti Star VX Hydrae[J]. ASTROPHYSICAL JOURNAL,2018,861(2):96. |
| APA | Xue, HF.,Fu, JN.,Fox-Machado, L.,Shi, JR.,Zhou, YT.,...&Altamirano-Devora, L.(2018).Asteroseismology of the Double-mode High-amplitude delta Scuti Star VX Hydrae.ASTROPHYSICAL JOURNAL,861(2),96. |
| MLA | Xue, HF,et al."Asteroseismology of the Double-mode High-amplitude delta Scuti Star VX Hydrae".ASTROPHYSICAL JOURNAL 861.2(2018):96. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| Asteroseismology of （3160KB） | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | Application Full Text | |
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment