XMM-Newton confirmation of soft X-ray excess emission in clusters of galaxies - The discovery of O VII emission from an extended warm baryonic component

Astronomy and Astrophysics

Volumn 397, Issue 2, 2003, Pages 445-462

  Kaastra, J S ^a   Lieu, R ^b   Tamura, T ^a   Paerels, F B S ^c   Den Herder, J W ^a  

^a SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^b UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

^c Och Spine at New York Presbyterian Hospitals   (United States)

Author keywords

Galaxies: clusters: general; Galaxies: cooling flows; X rays: galaxies: clusters

Indexed keywords

ELECTRONS; GASES; LIGHT EMISSION; MAGNETIC FIELDS; MICROWAVES; PLASMAS; RELATIVITY; SATELLITE OBSERVATORIES; SPECTRUM ANALYSIS; THERMAL EFFECTS; X RAYS;

GALACTIC FOREGROUND EMISSION; NEWTON CONFIRMATION; NONTHERMAL EMISSION MAGNETIC RECONNECTION; PLASMA COMPONENT; RELATIVISTIC ELECTRONS; SOFT X RAY EMISSION; THERMAL EMISSION; WARM BARYONIC COMPONENT; WARM HOT INTERGALACTIC MEDIUM;

GALAXIES;

EID: 0037240322     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20021514     Document Type: Article

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