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- W2074585149 abstract "We present a high-resolution radio study of the supernova remnant (SNR) G11.2-0.3 using archival Very Large Array data. Spectral tomography is performed to determine the properties of this composite-type SNR's individual components, which have only recently been distinguished through X-ray observations. Our results indicate that the spectral index of the pulsar wind nebula (PWN), or plerion, is αP = 0.25. We observe a spectral index of αS = 0.56 ± 0.02 throughout most of the SNR shell region but also detect a gradient in α in the southeastern component. We compare the spectral index and flux density with recent single-dish radio data of the source. Also, the radio efficiency and morphological properties of this PWN are found to be consistent with results for other known PWN systems." @default.
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- W2074585149 date "2002-06-10" @default.
- W2074585149 modified "2023-09-26" @default.
- W2074585149 title "Spectral Components of the Radio Composite Supernova Remnant G11.2−0.3" @default.
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- W2074585149 doi "https://doi.org/10.1086/340229" @default.
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