Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Shiyan Zhong"'
Autor:
Xinlei Chen, Brajesh Kumar, Xinzhong Er, Helong Guo, Yuan-Pei Yang, Weikang Lin, Yuan Fang, Guowang Du, Chenxu Liu, Jiewei Zhao, Tianyu Zhang, Yuxi Bao, Xingzhu Zou, Yu Pan, Yu Wang, Xufeng Zhu, Kaushik Chatterjee, Xiangkun Liu, Dezi Liu, Edoardo P. Lagioia, Geeta Rangwal, Shiyan Zhong, Jinghua Zhang, Jianhui Lian, Yongzhi Cai, Yangwei Zhang, Xiaowei Liu
Publikováno v:
The Astrophysical Journal Letters, Vol 971, Iss 1, p L2 (2024)
We present early-phase good-cadence (hour-to-day) simultaneous multiband ( ugi and vrz bands) imaging of the nearby supernova SN 2024ggi, which exploded in the nearby galaxy NGC 3621. A quick follow-up was conducted within less than a day after the e
Externí odkaz:
https://doaj.org/article/9e758fda25914355a1a05a30446d5b0f
Autor:
Dong-Wei Bao, Wei-Jian Guo, Zhi-Xiang Zhang, Cheng Cheng, Zhu-Heng Yao, Yan-Rong Li, Ye-Fei Yuan, Sui-Jian Xue, Jian-Min Wang, Chao-Wei Tsai, Hu Zou, Yong-Jie Chen, Wenxiong Li, Shiyan Zhong, Zhi-Qiang Chen
Publikováno v:
The Astrophysical Journal, Vol 977, Iss 2, p 279 (2024)
We present a noteworthy transient AT 2021aeuk exhibiting three distinct optical flares between 2018 and 2023. It is hosted in a radio-loud narrow-line Seyfert 1 galaxy, with an optical image showing a minor tidal morphology and a red mid-infrared col
Externí odkaz:
https://doaj.org/article/adf01f1cba69466c89ad8746be85f2d3
Publikováno v:
The Astrophysical Journal, Vol 959, Iss 1, p 19 (2023)
Tidal disruption events (TDEs) provide a clue to the properties of a central supermassive black hole (SMBH) and an accretion disk around it, and to the stellar density and velocity distributions in the nuclear star cluster surrounding the SMBH. Devia
Externí odkaz:
https://doaj.org/article/7e247fb23e874c9f84de583922417e19
Publikováno v:
The Astrophysical Journal, Vol 944, Iss 1, p 109 (2023)
By using direct N -body numerical simulations, we model the dynamical coevolution of two supermassive black holes (SMBHs) and the surrounding stars in merging galaxies. In order to investigate how different stellar components evolve during the merger
Externí odkaz:
https://doaj.org/article/99c3f09093ae4ae5a4ff5d002e877125
The capture of compact objects by massive black holes in galaxies or dwarf galaxies will generate short gravitational wave signals, called extreme-mass-ratio bursts (EMRBs), before evolving into extreme-mass-ratio inspirals. Their detection will prov
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2eb684e1a71e95ecdebd66d83914fb71
http://arxiv.org/abs/2209.13387
http://arxiv.org/abs/2209.13387
Publikováno v:
The Astrophysical Journal. 933:96
Tidal disruption of stars in dense nuclear star clusters containing supermassive central black holes (SMBH) is modeled by high-accuracy direct N-body simulation. Stars getting too close to the SMBH are tidally disrupted and a tidal disruption event (
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::677f4989e3bced963bceedce5ec3ea05
https://doi.org/10.3847/1538-4357/ac71ad
https://doi.org/10.3847/1538-4357/ac71ad
Autor:
Victoria Wang, Shiyan Zhong, Edina C. Wang, Jun Xia, Wei Chen, Xiao Ye Su, Ruizhen Xu, Guoping Sun
Publikováno v:
Advances in Radiation Oncology
Purpose The current situation of coronavirus disease 2019 (COVID-19) is rapidly evolving. Radiation therapy facilities are places of concentrated patient interactions. Oncology patients with immunosuppression are at a higher risk for contracting seve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a143a22bd0120ee2d7a9ad02b996ceca
https://pubmed.ncbi.nlm.nih.gov/32292840
https://pubmed.ncbi.nlm.nih.gov/32292840
Publikováno v:
Proceedings of the International Astronomical Union. 10:109-112
Tidal Disruption (TD) of stars by supermassive central black holes from dense rotating star clusters is modeled by high-accuracy direct N-body simulation. We study the time evolution of the stellar tidal disruption rate and the origin of tidally disr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::72d5a3fa79c38d0f7dc3788ddd52351d
https://doi.org/10.1017/s1743921315007632
https://doi.org/10.1017/s1743921315007632
Publikováno v:
The Astrophysical Journal. 855:129
We study the rates of tidal disruption of stars by intermediate-mass to supermassive black holes on bound to unbound orbits by using high-accuracy direct N-body experiments. The approaching stars from the star cluster to the black hole can take three
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3a3da130109281dff4dd67e1a5141e6
https://doi.org/10.3847/1538-4357/aab0a5
https://doi.org/10.3847/1538-4357/aab0a5
Autor:
Hui Sun, YouJun Lu, Zhu Liu, Feng Yuan, Zhuo Li, Wei-Hua Lei, FuKun Liu, Junfeng Wang, Tinggui Wang, ShiYan Zhong, YiZhong Fan, Xian Chen, LiXin Li, Hongyan Zhou, Weimin Yuan, Shuo Li
Publikováno v:
SCIENTIA SINICA Physica, Mechanica & Astronomica. 48:039503
When a star enters the tidal radius of a massive black hole (BH) at the center of a galaxy, the tidal force will rip the star apart. The BH may accrete the debris of the star and produce energetic flare. This phenomenon is now commonly known as Tidal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d082a0469589e15c3e0ce305df67962b
https://doi.org/10.1360/sspma2017-00268
https://doi.org/10.1360/sspma2017-00268