The nature of the X-ray halo of the plerion G21.5-0.9 unveiled by XMM-Newton and Chandra

Astronomy and Astrophysics

Volumn 442, Issue 2, 2005, Pages 539-548

  Bocchino, F ^a   Van Der Swaluw, E ^b,c   Chevalier, R ^d   Bandiera, R ^e  

^a INAF OSSERVATORIO ASTRONOMICO DI PALERMO   (Italy)

^b FOM INSTITUTE FOR PLASMA PHYSICS RIJNHUIZEN   (Netherlands)

^c UNIVERSITY OF LEEDS   (United Kingdom)

^d UNIVERSITY OF VIRGINIA   (United States)

^e INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

ISM: dust, extinction; ISM: supernova remnants; Radiation mechanisms: non thermal; Stars: supernovae: general; X rays: individuals: G21.5 0.9; X rays: ISM

Indexed keywords

ASTRONOMY; DATA REDUCTION; DIFFUSION; GAS EMISSIONS; X RAYS;

ISM: DUST, EXTINCTION; ISM: SUPERNOVA REMNANTS; STARS: SUPERNOVAE: GENERAL; STRAS: RADIATION MECHANISMS: NON-THERMAL; X-RAY: ISM; X-RAYS: INDIVUDUALS: G21.5-0.9;

ASTROPHYSICS;

EID: 27144501852     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20052870     Document Type: Article

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