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Pinwheel Outflow Induced by Stellar Mass Loss in a Coplanar Triple System
Kim, Hyosun1; Morris, Mark R.2; Kim, Jongsoo1; He JH(何金华)3,4,5
发表期刊ASTROPHYSICAL JOURNAL
2024-05-01
卷号966期号:2
DOI10.3847/1538-4357/ad34b9
产权排序第3完成单位
收录类别SCI
摘要We develop a physical framework for interpreting complex circumstellar patterns whorled around asymptotic giant branch (AGB) stars by investigating stable, coplanar triple systems using hydrodynamic and particle simulations. The introduction of a close tertiary body causes an additional periodic variation in the orbital velocity and trajectory of the AGB star. As a result, the circumstellar outflow builds a fine non-Archimedean spiral pattern superimposed upon the Archimedean spiral produced by the outer binary alone. This fine spiral can be approximated by off-centered circular rings that become tangent to each other at the location of the Archimedean spiral. The superimposed fine pattern fades out relatively quickly as a function of distance from the center of the system, in contrast to the dominant Archimedean spiral pattern, which presents a much slower fractional density decrease with radius. The different rates of radial decrease of the density contrast in the two superimposed patterns, coupled with their different time and spatial scales, lead to an apparent, but illusory radial change in the observed pattern interval, as has been reported, for example, in CW Leo. The function describing the detailed radial dependence of the expansion velocity is different in the two patterns, which may be used to distinguish them. The shape of the circumstellar whorled pattern is further explored as a function of the orbital eccentricity and the inner companion's mass. Although this study is confined to stable, coplanar triple systems, the results are likely applicable to moderately noncoplanar systems and open interesting avenues for studying noncoplanar systems.
资助项目National Research Foundation of Korea (NRF)https://doi.org/10.13039/501100003725[NRF-2021R1A2C1008928]; National Research Foundation of Korea (NRF) grant[2023-1-840-00]; Korea Astronomy and Space Science Institute (KASI); Korean government (MSIT)[11873086]; NSFC project; Chinese Academy of Sciences (CAS); CAS South America Center for Astronomy (CASSACA) in Santiago, Chile
项目资助者National Research Foundation of Korea (NRF)https://doi.org/10.13039/501100003725[NRF-2021R1A2C1008928] ; National Research Foundation of Korea (NRF) grant[2023-1-840-00] ; Korea Astronomy and Space Science Institute (KASI) ; Korean government (MSIT)[11873086] ; NSFC project ; Chinese Academy of Sciences (CAS) ; CAS South America Center for Astronomy (CASSACA) in Santiago, Chile
语种英语
学科领域天文学 ; 恒星与银河系
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS记录号WOS:001221149800001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]PLANETARY-NEBULAE ; PREPLANETARY NEBULAE ; CENTRAL STAR ; BINARY ; COMPANIONS ; WIND ; EVOLUTION ; ENVELOPE ; PATTERN ; PERTURBATIONS
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被引频次:1[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/27368
专题其他
作者单位1.Korea Astronomy and Space Science Institute, 776 Daedeok-daero, Yuseong-gu, Daejeon 34055, Republic of Korea; [email protected];
2.Department of Physics and Astronomy, University of California, Los Angeles, CA 90095-1547, USA;
3.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, People's Republic of China;
4.Chinese Academy of Sciences South America Center for Astronomy, National Astronomical Observatories, CAS, Beijing 100101, People's Republic of China;
5.Departamento de Astronomía, Universidad de Chile, Casilla 36-D, Santiago, Chile
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Kim, Hyosun,Morris, Mark R.,Kim, Jongsoo,et al. Pinwheel Outflow Induced by Stellar Mass Loss in a Coplanar Triple System[J]. ASTROPHYSICAL JOURNAL,2024,966(2).
APA Kim, Hyosun,Morris, Mark R.,Kim, Jongsoo,&何金华.(2024).Pinwheel Outflow Induced by Stellar Mass Loss in a Coplanar Triple System.ASTROPHYSICAL JOURNAL,966(2).
MLA Kim, Hyosun,et al."Pinwheel Outflow Induced by Stellar Mass Loss in a Coplanar Triple System".ASTROPHYSICAL JOURNAL 966.2(2024).
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