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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
We present new observations of the field centered on X-ray source 1E 1547.0-5408. Analysis of a new Chandra observation shows that it is unresolved at arcsecond resolution, and analysis of a new XMM-Newton observation shows that its X-ray spectrum is best described by an absorbed power-law and blackbody model. A …