8–13 Sept 2019
Europe/Rome timezone
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X-rays, SZ and Optical joint analysis of the hot and diffuse baryons within the Planck-detected triple-cluster systems

13 Sept 2019, 16:36
2m

Speaker

Mr Edouard Lecoq (IAS, CNRS/Université Paris-Sud, Université Paris-Saclay, Orsay CEDEX, France)

Description

Recent stacking analysis of Sunyaev-Zel'dovich (SZ) oberservations of hundreds of superclusters have revealed the presence of the warm-hot intergalactic medium (WHIM) as a component of the intercluster gas. This indicates that superclusters are good targets to directly study the WHIM.

We are conducting a detailed study of two triple-cluster systems detected by Planck. We will jointly analyse the SZ data from Planck together with X-rays and galaxy distribution observations with XMM-Newton and VTL/FORS2 respectively. We will present the supercluster components including a possible direct detection of WHIM. We will discuss their physical properties (e.g. temperature, density, pressure, entropy) and their impact on the missing baryon problem.

Affiliation IAS, CNRS/Université Paris-Sud, Université Paris-Saclay, Orsay CEDEX, France
Topic Hot and diffuse baryons

Primary author

Mr Edouard Lecoq (IAS, CNRS/Université Paris-Sud, Université Paris-Saclay, Orsay CEDEX, France)

Co-authors

Dr Alexander Kolodzig (IAS, CNRS/Université Paris-Sud, Université Paris-Saclay, Orsay CEDEX, France) Dr Nabila Aghanim (IAS, CNRS/Université Paris-Sud, Université Paris-Saclay, Orsay CEDEX, France) Prof. Mathieu Langer (IAS, CNRS/Université Paris-Sud, Université Paris-Saclay, Orsay CEDEX, France) Dr Marian Douspis (IAS, CNRS/Université Paris-Sud, Université Paris-Saclay, Orsay CEDEX, France) Mr Victor Bonjean (IAS, CNRS/Université Paris-Sud, Université Paris-Saclay, Orsay CEDEX, France) Dr Etienne Pointecouteau (IRAP, Université de Toulouse, CNRS, CNES, UPS, Toulouse, France* )

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