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Volumn 487, Issue 3, 2008, Pages 1033-1040
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High resolution radio study of the pulsar wind nebula within the supernova remnant G0.9+0.1
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Author keywords
ISM: individual objects: G0.9+0.1; ISM: supernova remnants; Radio continuum: ISM; X rays: ISM
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Indexed keywords
ACOUSTIC INTENSITY;
ESTIMATION;
IMAGE ENHANCEMENT;
IMAGING TECHNIQUES;
PHOTOGRAPHY;
POWDERS;
SIGNAL TO NOISE RATIO;
ANGULAR RESOLUTIONS;
ARCHIVAL DATA;
AUSTRALIA;
CHANDRA;
COMPACT ARRAYS;
COMPACT CORE;
FLUX DENSITIES;
HIGH RESOLUTIONS;
HIGH-FIDELITY IMAGES;
ISM: INDIVIDUAL OBJECTS: G0.9+0.1;
ISM: SUPERNOVA REMNANTS;
MULTICONFIGURATION;
NEUTRON STARS;
OBSERVATIONAL DATA;
PULSAR WIND NEBULAE;
RADIO CONTINUUM: ISM;
RADIO DATA;
RADIO EMISSIONS;
RADIO FREQUENCIES;
RADIO RANGE;
RADIO WAVELENGTHS;
RICH STRUCTURE;
SPATIAL SCALING;
SPECTRAL INDEX;
SUPERNOVA REMNANTS;
X-RAY DATA;
X-RAY IMAGING;
X-RAYS: ISM;
X RAYS;
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EID: 49749146732
PISSN: 00046361
EISSN: 14320746
Source Type: Journal
DOI: 10.1051/0004-6361:200809987 Document Type: Article |
Times cited : (39)
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References (23)
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