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Evidence for Non-Hydrostatic Gas Motions in the...
Preprint

Evidence for Non-Hydrostatic Gas Motions in the Hot ISM of Centaurus A

Abstract

We present preliminary results from a deep (600 ks) {\em Chandra} observation of the hot interstellar medium of the nearby early-type galaxy Centaurus A (Cen

Authors

Kraft RP; Hardcastle MJ; Sivakoff GR; Jordán A; Nulsen PEJ; Birkinshaw M; Forman WR; Jones C; Worrall DM; Croston JH

Publication date

March 25, 2008

DOI

10.48550/arxiv.0803.3595

Preprint server

arXiv