Temperature Structure in Abell 1367

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Temperature Structure in Abell 1367

We study the temperature structure of the rich cluster of galaxies Abell 1367 using two independent methods of correcting for the ASCA PSF. The results of the two methods are in excellent agreement and give solid evidence of a strong and localized shock in the intracluster medium (ICM). Our analysis suggests that we are observing the merger of two subclusters. We find that the lower luminosity ...

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ژورنال

عنوان ژورنال: The Astrophysical Journal

سال: 1998

ISSN: 0004-637X,1538-4357

DOI: 10.1086/305719