中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Pulsations of Three Rapidly Oscillating Ap Stars TIC 96315731, TIC 72392575, and TIC 318007796

文献类型:期刊论文

作者Zhong, Hai-Jian1; Shen, Dong-Xiang1; Zhu, Chun-Hua1; Liu, He-Lei1; Guo, Su-Fen1; Lu, Guo-Liang2
刊名RESEARCH IN ASTRONOMY AND ASTROPHYSICS
出版日期2024-08-01
卷号24期号:8页码:085014
关键词asteroseismology techniques: photometric stars: oscillations (including pulsations) stars: chemically peculiar
ISSN号1674-4527
DOI10.1088/1674-4527/ad621d
产权排序2
英文摘要We analyze the frequencies of three known roAp stars, TIC 96315731, TIC 72392575, and TIC 318007796, using the light curves from the Transiting Exoplanet Survey Satellite. For TIC 96315731, the rotational and pulsational frequencies are 0.1498360 day(-1) and 165.2609 day(-1), respectively. In the case of TIC 72392575, the rotational frequency is 0.25551 day(-1). We detect a quintuplet of pulsation frequencies with a center frequency of 135.9233 day(-1), along with two signals within the second pair of rotational sidelobes of the quintuplet separated by the rotation frequency. These two signals may correspond to the frequencies of a dipole mode. In TIC 318007796, the rotational and pulsational frequencies are 0.2475021 day(-1), 192.73995 day(-1), and 196.33065 day(-1), respectively. Based on the oblique pulsator model, we calculate the rotation inclination (i) and magnetic obliquity angle (beta) for the stars, which provide the geometry of the pulsation modes. Combining the phases of the frequency quintuplets, the pulsation amplitude and phase modulation curves, and the results of spherical harmonic decomposition, we conclude that the pulsation modes of frequency quintuplets in TIC 96315731, TIC 72392575, and TIC 318007796 correspond to distorted dipole mode, distorted quadrupole mode, and distorted dipole mode, respectively.
WOS关键词DISTORTED DIPOLE MODE ; MAGNETIC-FIELDS ; ROAP STARS ; CATALOG ; DISCOVERY ; PECULIAR ; ROTATION
资助项目NASA Explorer Program ; National Natural Science Foundation of China (NSFC)[U2031204] ; National Natural Science Foundation of China (NSFC)[12373038] ; National Natural Science Foundation of China (NSFC)[12163005] ; National Natural Science Foundation of China (NSFC)[12288102] ; China Manned Space Project[CMSCSST-2021-A10] ; Natural Science Foundation of Xinjiang[2022D01D85] ; Natural Science Foundation of Xinjiang[2022TSYCLJ0006]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001291501200001
出版者NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
资助机构NASA Explorer Program ; National Natural Science Foundation of China (NSFC) ; China Manned Space Project ; Natural Science Foundation of Xinjiang
源URL[http://ir.xao.ac.cn/handle/45760611-7/6914]  
专题研究单元未命名
通讯作者Zhu, Chun-Hua; Lu, Guo-Liang
作者单位1.Xinjiang Univ, Sch Phys Sci & Technol, Urumqi 830046, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, Natl Astron Observ, Urumqi 830000, Peoples R China
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Zhong, Hai-Jian,Shen, Dong-Xiang,Zhu, Chun-Hua,et al. Pulsations of Three Rapidly Oscillating Ap Stars TIC 96315731, TIC 72392575, and TIC 318007796[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2024,24(8):085014.
APA Zhong, Hai-Jian,Shen, Dong-Xiang,Zhu, Chun-Hua,Liu, He-Lei,Guo, Su-Fen,&Lu, Guo-Liang.(2024).Pulsations of Three Rapidly Oscillating Ap Stars TIC 96315731, TIC 72392575, and TIC 318007796.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,24(8),085014.
MLA Zhong, Hai-Jian,et al."Pulsations of Three Rapidly Oscillating Ap Stars TIC 96315731, TIC 72392575, and TIC 318007796".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 24.8(2024):085014.

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