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-Reference-Cited by-同舟云学术

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

Published:2007-10 Issue:2 Volume:667 Page:1111-1118
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Gelfand Joseph D.,Gaensler B. M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference62 articles.

1. GLIMPSE. I. AnSIRTFLegacy Project to Map the Inner Galaxy

2. SUMSS: A Wide-Field Radio Imaging Survey of the Southern Sky. I. Science Goals, Survey Design, and Instrumentation

3. SwiftandChandraconfirm the intensity-hardness correlation of the AXP 1RXS J170849.0–400910

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