A multiwavelength study of the radio source G296.7−0.9: confirmation as a Galactic supernova remnant (original) (raw)

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Monthly Notices of the Royal Astronomical Society, 2006

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On the origin of the jet-like radio/X-ray morphology of G290.1–0.8

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Accepted by The Astrophysical Journal Preprint typeset using LATEX style emulateapj v. 5/2/11 HIGH-ENERGY EMISSION FROM THE COMPOSITE SUPERNOVA REMNANT MSH 15–56

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The Compact X‐Ray Source 1E 1547.0−5408 and the Radio Shell G327.24‐0.13: A New Proposed Association between a Candidate Magnetar and a Candidate Supernova Remnant

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