Fe K α line emission from the Arches cluster region - Evidence for ongoing particle bombardment?

Astronomy and Astrophysics

Volumn 530, Issue , 2011, Pages

  Capelli, R ^a   Warwick, R S ^b   Porquet, D ^c   Gillessen, S ^a   Predehl, P ^a  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b UNIVERSITY OF LEICESTER   (United Kingdom)

^c UNIVERSITÉ DE STRASBOURG   (France)

Author keywords

Cosmic rays; Galaxy: center; ISM: clouds

Indexed keywords

BACKGROUND SUBTRACTION; CLUSTER REGIONS; COSMIC-RAY PARTICLES; EDGE FEATURES; FE-K EDGE; FLUENCES; GALACTIC CENTER; GALACTIC CENTER REGION; GALAXY: CENTER; ISM: CLOUDS; LIGHTCURVES; LINE EMISSIONS; MOLECULAR CLOUDS; MOLECULAR COMPLEXES; MOLECULAR KNOTS; NARROW ENERGY BANDS; NONTHERMAL; OBSERVATION WINDOW; PARTICLE BOMBARDMENT; SPECTRAL FITTING; TEMPORAL BEHAVIOUR; TIME-AVERAGED; TIME-SCALES; X RAY FLUORESCENCE; X RAY PHOTONS; X-RAY CONTINUUM; X-RAY SOURCES; XMM-NEWTON OBSERVATIONS;

ARCHES; COSMIC RAYS; COSMOLOGY; FLUORESCENCE; GALAXIES; PHOTONS; X RAYS;

CLOUDS;

EID: 79955605812     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201116574     Document Type: Article

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