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- W47774687 abstract "We present bi-dimensional temperature and abundance analysis of the ICM by using archival data of ASCA. Spectrum best-fit result within a radius 12′ is a 7.2 ± 0.2 keV temperature value. This is consistent with the previous ASCA analysis of Nevalainen et. al. (6.9 ± 0.2 keV). Bidimensional temperature map shows a region with significantly lower temperature value (6.2 ± 0.5 keV) than the ICM average and with a remarkable cool trail-like shape in the northwest of the cluster. Equivalent-Width map also displays a high abundance region on the west side, which coincides with the head of the cool trail. Quintana & Souza (1993) indicates a north-south direction alignment in the galaxy number density map. We record a disturbance of the X-ray brightness map in the same direction. In addition to above all, having an extended optical halo of its central galaxy MCG05-33-002 (Kemp & Meaburn 1991) in the same direction suggests that -if the locations of peculiar regions are not a chance projectionA3571 is experiencing an ongoing subcluster merging: A subcluster is coming from northeast of the main cluster, penetrating in the ICM and leaving a cool trail -due to destructive effects like ram pressure strippingand a survived high abundance core for the present epoch." @default.
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- W47774687 date "2003-02-01" @default.
- W47774687 modified "2023-10-16" @default.
- W47774687 title "Analysis of Temperature and Abundance Distribution in Abell 3571: An Ongoing Subcluster Merging?" @default.
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