中文

KMT-2021-BLG-0322:三重透镜与高阶双星透镜解释之间的严重简并

地球与行星天体物理 2021-11-17 v1 星系天体物理 天体物理仪器与方法 太阳与恒星天体物理

摘要

我们研究了微引力透镜事件 KMT-2021-BLG-0322,其光变曲线表现出三组显著的焦散穿越特征。研究发现,光变曲线的整体特征可由双星透镜(2L1S)模型近似描述,但该模型留下了显著的残差。我们检验了多种旨在解释残差的解释。我们发现,残差既可以通过考虑由微透镜视差和透镜轨道效应引起的非直线透镜-源运动来解释,也可以通过向双星透镜添加一颗低质量伴星(3L1S 模型)来解释。高阶 2L1S 模型与 3L1S 模型之间的简并非常严重,难以基于测光数据挑出正确解。这一简并此前在另外两个事件(MACHO-97-BLG-41 和 OGLE-2013-BLG-0723)中已知,曾导致对双星系统中行星的误探测,因此 KMT-2021-BLG-0322 中该简并的识别表明,这种简并不仅可能常见,而且可能非常严重,强调了需要检验对偏离 2L1S 模型的两种解释。根据以事件时标、角爱因斯坦半径和微透镜视差等已测透镜可观测量进行的贝叶斯分析,估计对于 2L1S 和 3L1S 解,双星透镜成员质量均为 (M1,M2)=(0.620.26+0.25 M,0.070.03+0.03 M)(M_1, M_2) =(0.62^{+0.25}_{-0.26}~M_\odot,0.07^{+0.03}_{-0.03}~M_\odot),而根据 3L1S 解得到的第三透镜成员质量为 M3=6.402.78+2.64 MJM_3=6.40^{+2.64}_{-2.78}~M_{\rm J}

关键词

引用

@article{arxiv.2109.02210,
  title  = {KMT-2021-BLG-0322: Severe degeneracy between triple-lens and higher-order binary-lens interpretations},
  author = {Cheongho Han and Andrew Gould and Yuki Hirao and Chung-Uk Lee and Michael D. Albrow and Sun-Ju Chung and Kyu-Ha Hwang and Youn Kil Jung and Doeon Kim and Shude Mao and Yoon-Hyun Ryu and In-Gu Shin and Yossi Shvartzvald and Jennifer C. Yee and Weicheng Zang and Sang-Mok Cha and Dong-Jin Kim and Hyoun-Woo Kim and Seung-Lee Kim and Dong-Joo Lee and Yongseok Lee and Byeong-Gon Park and Richard W. Pogge and Fumio Abe and Richard Barry and David P. Bennett and Aparna Bhattacharya and Ian Bond and Martin Donachie and Hirosane Fujii and Akihiko Fukui and Yoshitaka Itow and Rintaro Kirikawa and Iona Kondo and Naoki Koshimoto and Man Cheung Alex Li and Yutaka Matsubara and Yasushi Muraki and Shota Miyazaki and Clément Ranc and Nicholas J. Rattenbury and Yuki Satoh and Hikaru Shoji and Takahiro Sumi and Daisuke Suzuki and Yuzuru Tanaka and Paul J. Tristram and Tsubasa Yamawaki and Atsunori Yonehara},
  journal= {arXiv preprint arXiv:2109.02210},
  year   = {2021}
}

备注

9 pages, 10 figures, 3 tables