Cool core remnants in galaxy clusters*

Author： Rossetti M.   Molendi S.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|510|issue|A83-A83

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.510, Iss.issue, 2010-02, pp. : A83-A83

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

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Abstract

Context. X ray clusters are conventionally divided into two classes: “cool core” (CC) and “non-cool core” (NCC) objects, on the basis of the observational properties of their central regions. Recent results have shown that the cluster population is bimodal.

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