XMM-Newton high-resolution spectroscopy reveals the chemical evolution of M 87

Astronomy and Astrophysics

Volumn 459, Issue 2, 2006, Pages 353-360

  Werner, N ^a   Bohringer H ^c   Kaastra, J S ^a   De Plaa, J ^a,b   Simionescu, A ^c   Vink, J ^b  

^a SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^b UTRECHT UNIVERSITY   (Netherlands)

^c MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

Cooling flows; Galaxies: abundances; Galaxies: individual: M 87; Galaxies: intergalactic medium; Galaxies: ISM; X rays: galaxies: clusters

Indexed keywords

CARBON; DIFFRACTION GRATINGS; ELECTROMAGNETIC WAVE REFLECTION; NITROGEN; OPTICAL RESOLVING POWER; OXYGEN; SPECTROSCOPIC ANALYSIS;

COOLING FLOWS; GALAXIES: ABUNDANCES; GALAXIES: INDIVIDUAL: M 87; GALAXIES: INTERGALACTIC MEDIUMS; X-RAYS: GALAXIES: CLUSTERS;

GALAXIES;

EID: 33751017096     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20065678     Document Type: Article

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