Tidal disruption events and quasi-periodic eruptions

被引:2
|
作者
Webb, Natalie A. [1 ]
Barret, Didier [1 ]
Godet, Olivier [1 ]
Gupta, Maitrayee [1 ]
Lin, Dacheng [2 ]
Quintin, Erwan [1 ]
Tranin, Hugo [1 ]
机构
[1] Univ Toulouse, Inst Rech Astrophys & Planetol, CNRS, CNES, Toulouse, France
[2] Univ New Hampshire, Space Sci Ctr, Durham, NH USA
基金
欧盟地平线“2020”;
关键词
x-rays; galaxies; nuclei; dwarf; catalogs; MASS BLACK-HOLE; FOLLOW-UP OBSERVATIONS; X-RAY FLARE; ESO; 243-49; SOLAR MASSES; STARS; GALAXY; DISK; MULTIWAVELENGTH; ENVIRONMENT;
D O I
10.1002/asna.20230051
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Tidal disruption events (TDEs) occur when a star passes close to a massive black hole so that the tidal forces of the black hole exceed the binding energy of a star and cause it to be ripped apart. Part of the matter will fall onto the black hole, causing a strong increase in luminosity. Such events are often seen in the optical or the x-ray (or both) or even at other wavelengths such as in the radio, where the diversity of observed emission is still poorly understood. The XMM-Newton catalog of approximately a million x-ray detections covering 1283(2) degrees of sky contains a number of these events. Here I will show the diverse nature of a number of TDEs discovered in the catalog and discuss their relationship with quasi-periodic eruptions.
引用
收藏
页数:7
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