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- W2077115443 abstract "High-resolution radio observations of the nuclear region of Luminous and Ultraluminous Infrared Galaxies (ULIRGs) have shown that its radio structure consists of a compact high surface-brightness central radio source inmersed in a diffuse low brightness circumnuclear halo. While the central component could be associated with an AGN or compact star-forming regions where radio supernovae are exploding, it is well known that the circumnuclear regions host bursts of star-formation. The studies of radio supernovae can provide essential information about stellar evolution and CSM/ISM properties in regions hidden by dust at optical and IR wavelengths. In this contribution, we show results from radio interferometric observations from NGC 7469, IRAS 18293-3413 and IRAS 17138-1017 where three extremely bright radio supernovae have been found. High-resolution radio observations of these and other LIRGs would allow us to determine the core-collapse supernova rate in them as well as their star-formation rate." @default.
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- W2077115443 date "2008-10-01" @default.
- W2077115443 modified "2023-10-16" @default.
- W2077115443 title "High resolution radio observations of nuclear and circumnuclear regions of luminous infrared galaxies (LIRGs)" @default.
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- W2077115443 doi "https://doi.org/10.1088/1742-6596/131/1/012037" @default.
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