Morphology and 2D-temperature distribution of the x-ray emitting gas in galaxy 
clusters, measured with XMM-Newton

Briel, Ulrich G.; Finoguenov, Alexis; Henry, Patrick J.

Item

ITEM ACTIONSEXPORT

Add to Basket

Local TagsRelease HistoryDetailsSummary

Released

Conference Paper

Morphology and 2D-temperature distribution of the x-ray emitting gas in galaxy clusters, measured with XMM-Newton

MPS-Authors

Briel, Ulrich G.
Max Planck Society;

/persons/resource/persons16183

Finoguenov, Alexis
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

External Resource

No external resources are shared

Fulltext (restricted access)

There are currently no full texts shared for your IP range.

Fulltext (public)

There are no public fulltexts stored in PuRe

Supplementary Material (public)

There is no public supplementary material available

Citation

Briel, U. G., Finoguenov, A., & Henry, P. J. (2003). Morphology and 2D-temperature distribution of the x-ray emitting gas in galaxy clusters, measured with XMM-Newton. In T. Ohashi, & N. Yamasaki (Eds.), Workshop on Galaxies and Clusters of Galaxies (pp. 149-154). Tokyo: Japan society for promotion of science.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-E700-F

Abstract

There is no abstract available