Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006

Astronomy and Astrophysics

Volumn 501, Issue 1, 2009, Pages 239-249

  Miceli, M ^a,b,c   Bocchino, F ^b,c   Iakubovskyi, D ^d   Orlando, S ^b,c   Telezhinsky, I ^e   Kirsch, M G F ^f   Petruk, O ^c,g,h   Dubner, G ⁱ   Castelletti, G ⁱ  

^a UNIVERSITY OF PALERMO   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^c Consorzio COMETA ^*  (Italy)

^d BOGOLYUBOV INSTITUTE FOR THEORETICAL PHYSICS   (Ukraine)

^e TARAS SHEVCHENKO NATIONAL UNIVERSITY OF KYIV   (Ukraine)

^f ESA ESOC   (Germany)

^g PIDSTRYHACH INSTITUTE FOR APPLIED PROBLEMS OF MECHANICS AND MATHEMATICS   (Ukraine)

^h IVAN FRANKO NATIONAL UNIVERSITY OF LVIV   (Ukraine)

ⁱ INSTITUTO DE ASTRONOMÍA Y FÍSICA DEL ESPACIO   (Argentina)

Author keywords

ISM: individual objects: SN 1006; ISM: supernova remnants; X rays: ISM

Indexed keywords

ASPECT ANGLES; AZIMUTHAL VARIATIONS; CHEMICAL COMPOSITIONS; COMBINED ANALYSIS; CONTACT DISCONTINUITIES; ENERGY BAND; INTERSTELLAR MAGNETIC FIELDS; ISM: INDIVIDUAL OBJECTS: SN 1006; ISM: SUPERNOVA REMNANTS; LINE OF SIGHT; MHD MODELS; NONTHERMAL; NONTHERMAL EMISSION; PARTICLE ACCELERATION; PHYSICAL AND CHEMICAL PROPERTIES; SHOCK FRONTS; SPATIAL DISTRIBUTION; SPATIALLY RESOLVED; SPECTRAL ANALYSIS; SUPERNOVA REMNANTS; THERMAL EMISSIONS; THERMAL IMAGES; THERMAL X-RAYS; X RAY SPECTRUM; X-RAY EMITTING; X-RAY EMITTING PLASMAS; X-RAYS: ISM; XMM-NEWTON;

CHEMICAL PROPERTIES; EMISSION SPECTROSCOPY; MAGNETIC FIELDS; PARTICLE ACCELERATOR ACCESSORIES; SIZE DISTRIBUTION; SPECTRUM ANALYSIS; SPECTRUM ANALYZERS; THREE DIMENSIONAL;

X RAYS;

EID: 67651046506     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811505     Document Type: Article

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