中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Superoutbursts and Positive Superhumps Occurred during the Standstill of a Z Cam-type Dwarf Nova

文献类型:期刊论文

作者Sun, Qi-Bin3,4; Qian, Sheng-Bang3,4; Zhu LY(朱俐颖)1,2; Li, Qin-Mei3,4; Li FX(李福兴)2,4; Li MY(李敏榆)1,2; Li P(李平)1,2
刊名ASTROPHYSICAL JOURNAL
出版日期2025-04-01
卷号982期号:2
ISSN号0004-637X
DOI10.3847/1538-4357/adb7d9
产权排序第3完成单位
文献子类Article
英文摘要Dwarf novae (DNe) are semidetached binaries, where a white dwarf accretes material from a cool main-sequence companion via an accretion disk, and are known for their intermittent outbursts, making them key systems for studying accretion physics. The accumulation of large survey data sets has challenged traditional models, which assumed that the disk remains hot and cannot produce superoutbursts during the standstill of a Z Camelopardalis (Z Cam)-type DN and that superoutbursts require a mass ratio of q = M2/M1 <= 0.25-0.33. Here we report the detection of superoutbursts and positive superhumps (PSHs) during a standstill in the Z Cam-type star AT Cnc with a mass ratio larger than 0.33. Notably, the PSHs evolve gradually before the superoutburst begins, suggesting that an eccentric, precessing disk forms first, with the superoutburst occurring as the disk radius continues to expand. These findings provide the first detailed observational evidence of superoutbursts and PSHs occurring during standstill, offering important new insights into the classification of DNe and the underlying mechanisms of outbursts.
学科主题天文学 ; 恒星与银河系
URL标识查看原文
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
WOS关键词QUASI-PERIODIC OSCILLATIONS ; DISK INSTABILITY MODEL ; IW AND-TYPE ; MASS-TRANSFER ; NEGATIVE SUPERHUMPS ; ACCRETION DISKS ; VARIABLE-STARS ; HS 2325+8205 ; OUTBURSTS ; SIMULATIONS
资助项目MOST divided by National Key Research and Development Program of China (NKPs)https://doi.org/10.13039/501100012166[2022YFE0116800]; National Key R&D Program of China[11933008]; National Natural Science Foundation of China
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001450983200001
出版者IOP Publishing Ltd
资助机构MOST divided by National Key Research and Development Program of China (NKPs)https://doi.org/10.13039/501100012166[2022YFE0116800] ; National Key R&D Program of China[11933008] ; National Natural Science Foundation of China
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/28221]  
专题云南天文台_双星与变星研究组
作者单位1.University of Chinese Academy of Sciences, No.19(A) Yuquan Road, Shijingshan District, Beijing, People's Republic of China
2.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China;
3.Key Laboratory of Astroparticle Physics of Yunnan Province, Yunnan University, Kunming 650091, People's Republic of China;
4.Department of Astronomy, School of Physics and Astronomy, Yunnan University, Kunming 650091, People's Republic of China; qiansb@ynu.edu.cn;
推荐引用方式
GB/T 7714
Sun, Qi-Bin,Qian, Sheng-Bang,Zhu LY,et al. Superoutbursts and Positive Superhumps Occurred during the Standstill of a Z Cam-type Dwarf Nova[J]. ASTROPHYSICAL JOURNAL,2025,982(2).
APA Sun, Qi-Bin.,Qian, Sheng-Bang.,朱俐颖.,Li, Qin-Mei.,李福兴.,...&李平.(2025).Superoutbursts and Positive Superhumps Occurred during the Standstill of a Z Cam-type Dwarf Nova.ASTROPHYSICAL JOURNAL,982(2).
MLA Sun, Qi-Bin,et al."Superoutbursts and Positive Superhumps Occurred during the Standstill of a Z Cam-type Dwarf Nova".ASTROPHYSICAL JOURNAL 982.2(2025).

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来源:云南天文台

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