X-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary

The discrepancy between the optical and X-ray properties of tidal disruption events (TDE) is an unresolved issue. Here, the authors show delayed X-ray brightening after the optical flare in TDE OGLE16aaa followed by several flux dips during the decay phase that could be explained by the presence of...

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Autores principales:	Xinwen Shu, Wenjie Zhang, Shuo Li, Ning Jiang, Liming Dou, Zhen Yan, Fu-Guo Xie, Rongfeng Shen, Luming Sun, Fukun Liu, Tinggui Wang
Formato:	article
Lenguaje:	EN
Publicado:	Nature Portfolio 2020
Materias:	Science Q
Acceso en línea:	https://doaj.org/article/e9783b4f3aee4a0991246569a5991d3b
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spelling	oai:doaj.org-article:e9783b4f3aee4a0991246569a5991d3b2021-12-02T15:33:52ZX-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary10.1038/s41467-020-19675-z2041-1723https://doaj.org/article/e9783b4f3aee4a0991246569a5991d3b2020-11-01T00:00:00Zhttps://doi.org/10.1038/s41467-020-19675-zhttps://doaj.org/toc/2041-1723The discrepancy between the optical and X-ray properties of tidal disruption events (TDE) is an unresolved issue. Here, the authors show delayed X-ray brightening after the optical flare in TDE OGLE16aaa followed by several flux dips during the decay phase that could be explained by the presence of supermassive black hole binary or patchy obscuration.Xinwen ShuWenjie ZhangShuo LiNing JiangLiming DouZhen YanFu-Guo XieRongfeng ShenLuming SunFukun LiuTinggui WangNature PortfolioarticleScienceQENNature Communications, Vol 11, Iss 1, Pp 1-9 (2020)
institution	DOAJ
collection	DOAJ
language	EN
topic	Science Q
spellingShingle	Science Q Xinwen Shu Wenjie Zhang Shuo Li Ning Jiang Liming Dou Zhen Yan Fu-Guo Xie Rongfeng Shen Luming Sun Fukun Liu Tinggui Wang X-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary
description	The discrepancy between the optical and X-ray properties of tidal disruption events (TDE) is an unresolved issue. Here, the authors show delayed X-ray brightening after the optical flare in TDE OGLE16aaa followed by several flux dips during the decay phase that could be explained by the presence of supermassive black hole binary or patchy obscuration.
format	article
author	Xinwen Shu Wenjie Zhang Shuo Li Ning Jiang Liming Dou Zhen Yan Fu-Guo Xie Rongfeng Shen Luming Sun Fukun Liu Tinggui Wang
author_facet	Xinwen Shu Wenjie Zhang Shuo Li Ning Jiang Liming Dou Zhen Yan Fu-Guo Xie Rongfeng Shen Luming Sun Fukun Liu Tinggui Wang
author_sort	Xinwen Shu
title	X-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary
title_short	X-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary
title_full	X-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary
title_fullStr	X-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary
title_full_unstemmed	X-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary
title_sort	x-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary
publisher	Nature Portfolio
publishDate	2020
url	https://doaj.org/article/e9783b4f3aee4a0991246569a5991d3b
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X-ray flares from the stellar tidal disruption by a candidate supermassive black hole binary

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