Arxiv:2003.09066V1 [Astro-Ph.HE] 20 Mar 2020
DRAFT VERSION MARCH 23, 2020 Typeset using LATEX twocolumn style in AASTeX62 Multiwavelength Study of an X-ray Tidal Disruption Event Candidate in NGC 5092 DONGYUE LI,1, 2 R.D. SAXTON,3 WEIMIN YUAN,1, 2 LUMING SUN,4, 5 HE-YANG LIU,1, 2 NING JIANG,6, 5 HUAQING CHENG,1, 2 HONGYAN ZHOU,7, 5, 6 S. KOMOSSA,8, 9 AND CHICHUAN JIN1, 2 1Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100101, China 2School of Astronomy and Space Science, University of Chinese Academy of Sciences, 19A Yuquan Road, Beijing, 100049, China 3Telespazio-Vega UK for ESA, Euporean Space Astronomy Centre, Operations Department, E-28691 Villanueva de la Can~ada, Spain 4Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, The University of Science and Technology of China, Hefei, Anhui, 230026, China 5School of Astronomy and Space Sciences, University of Science and Technology of China, Hefei, Anhui, 230026, China 6Key laboratory for Research in Galaxies and Cosmology, Department of Astronomy, The University of Science and Technology of China, Hefei, Anhui, 230026, China 7Antarctic Astronomy Research Division, Key Laboratory for Polar Science of the State Oceanic Administration, Polar Research Institute of China, 451 Jinqiao Road, Shanghai, 20136, China 8Max Planck Institut fur¨ Radioastronomie, Auf dem Hugel¨ 69, D-53121 Bonn, Germany 9Key Laboratory of Space Science Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100101, China ABSTRACT We present multiwavelength studies of a transient X-ray source, XMMSL1 J131952.3+225958, associated with the galaxy NGC 5092 at z = 0:023 detected in the XMM-Newton SLew survey (XMMSL).
[Show full text]