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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Autores principales: Swartz, D.A., Pavlov, G.G., Clarke, T., Castelletti, G., Zavlin, V.E., Bucciantini, N., Karovska, M., Horst, A.J.V.D., Yukita, M., Weisskopf, M.C.
Formato: JOUR
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_0004637X_v808_n1_p_Swartz
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