Skip to main content
Go to the home page of the European Commission (opens in new window)
English en
CORDIS - EU research results
CORDIS
Content archived on 2024-05-29

The Cluster-Galaxy Connection: Interactions and Evolution

Objective

In the Universe, structure is formed hierarchically, by the merging of smaller units. Large clusters of galaxies are formed by the continual falling of galaxies into the clusters. The interactions of the cluster gas with the moving galaxies modify the pro perties of both galaxies and clusters by, for example, stripping the galaxies, and heating the cluster. These modifications have an impact on their subsequent evolution.I am proposing to combine my existing expertise in the analysis of X-ray data from evol ving and merging clusters of galaxies with MPIA's experience on deep galaxy surveys and galaxy dynamics in order to get a better insight into the factors that control the evolution of galaxies and clusters, and the impact of galaxy-cluster interactions. Su ch a combined study has not been done yet; it is timely, because of the availability of high quality X-ray data from the new satellites Chandra and XMM, and the wealth of ongoing deep galaxy surveys that are producing encouraging results.The properties of the clusters will be derived from the X-ray observations, while optical/infrared data will be used to find the galaxy characteristics. Appropriate methods for the handling of the X-ray and galaxy survey data have been developed and used by me and MPIA res pectively over the past years. Data already exist and the samples will be complimented when necessary by data from the rapidly expanding archives and/or after the submittion of proposals. My training will be on the use of large galaxy survey data, how to extract the essential information, and combine it successfully with the X-ray data. I also expect to gain a deeper knowledge on galaxy dynamics and galaxy interactions by being at MPIA.At the end of the project I will be able to assess the importance of ga laxy-cluster interactions in the modification of the properties and evolution of both clusters and galaxies, and the physical processes by which this occurs.

Fields of science (EuroSciVoc)

CORDIS classifies projects with EuroSciVoc, a multilingual taxonomy of fields of science, through a semi-automatic process based on NLP techniques. See: The European Science Vocabulary.

You need to log in or register to use this function

Keywords

Project’s keywords as indicated by the project coordinator. Not to be confused with the EuroSciVoc taxonomy (Fields of science)

Topic(s)

Calls for proposals are divided into topics. A topic defines a specific subject or area for which applicants can submit proposals. The description of a topic comprises its specific scope and the expected impact of the funded project.

Call for proposal

Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.

FP6-2002-MOBILITY-5
See other projects for this call

Funding Scheme

Funding scheme (or “Type of Action”) inside a programme with common features. It specifies: the scope of what is funded; the reimbursement rate; specific evaluation criteria to qualify for funding; and the use of simplified forms of costs like lump sums.

EIF - Marie Curie actions-Intra-European Fellowships

Coordinator

MAX-PLANCK-GESELLSCHAFT ZUR FOERDERUNG DER WISSENSCHAFTEN E.V.
EU contribution
No data
Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

No data
My booklet 0 0