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Chandra X-Ray Observations of G11.2–0.3: Implications for Pulsar Ages

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V. M. Kaspi1,2,3, M. E. Roberts1,2,4, G. Vasisht5, E. V. Gotthelf6, M. Pivovaroff7 and N. Kawai8,9

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A Multiwavelength Study on the High-energy Behavior of the Fermi/LAT Pulsars

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[Fe II] and H2 Filaments in the Supernova Remnant G11.2–0.3: Supernova Ejecta and Presupernova Circumstellar Wind

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J. W. T. Hessels et al.  The Astrophysical Journal 2004  612 389
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  1. Dense Iron Ejecta and Core-Collapse Supernova Explosion in the Young Supernova Remnant G11.2-0.3
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  3. The Pulsar Wind Nebula in G11.2–0.3

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