Wencheng Feng, Heng Yu, Haihui Zhao, Xiaolan Hou, Shumei Jia, Chengkui Li, Yulin Cheng, Paolo Tozzi, Ming Sun, Yong chen
{"title":"Weak Merging scenario of the CLASH Cluster A209","authors":"Wencheng Feng, Heng Yu, Haihui Zhao, Xiaolan Hou, Shumei Jia, Chengkui Li, Yulin Cheng, Paolo Tozzi, Ming Sun, Yong chen","doi":"10.1088/1674-4527/ad349a","DOIUrl":null,"url":null,"abstract":"\n We study the structural and dynamical properties of Abell 209 based on Chandra and XMM-Newton observations. We obtain detailed temperature, pressure and entropy maps with the contour binning method, and find a hot region in the NW direction. The X-ray brightness residual map and corresponding temperature profiles reveal a possible shock front in the NW direction and a cold front feature in the SE direction. Combing with the galaxy luminosity density map we propose a weak merger scenario. A young sub-cluster passing from the SE to NW direction could explain the optical subpeak, the ICM temperature map, the X-ray surface brightness excess, and the X-ray peak offset togethe.","PeriodicalId":509923,"journal":{"name":"Research in Astronomy and Astrophysics","volume":"26 48","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-03-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Research in Astronomy and Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1088/1674-4527/ad349a","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
We study the structural and dynamical properties of Abell 209 based on Chandra and XMM-Newton observations. We obtain detailed temperature, pressure and entropy maps with the contour binning method, and find a hot region in the NW direction. The X-ray brightness residual map and corresponding temperature profiles reveal a possible shock front in the NW direction and a cold front feature in the SE direction. Combing with the galaxy luminosity density map we propose a weak merger scenario. A young sub-cluster passing from the SE to NW direction could explain the optical subpeak, the ICM temperature map, the X-ray surface brightness excess, and the X-ray peak offset togethe.