HIGH SPATIAL RESOLUTION X-RAY SPECTROSCOPY of the IC 443 PULSAR WIND NEBULA and ENVIRONS

Deep Chandra ACIS observations of the region around the putative pulsar, CXOU J061705.3+222127, in the supernova remnant (SNR) IC 443 reveal an ∼5″ radius ring-like structure surrounding the pulsar and a jet-like feature oriented roughly north-south across the ring and through the pulsar's loca...

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Detalles Bibliográficos
Publicado:	2015
Materias:	ISM: individual objects (G189.22+2.90 IC 443) ISM: supernova remnants stars: neutron X-rays: individual (CXOU J061705.3+222127) X-rays: ISM
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v808_n1_p_Swartz http://hdl.handle.net/20.500.12110/paper_0004637X_v808_n1_p_Swartz
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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