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RGB composite image where the total intensity map of Raspberry, observed by ASKAP at ν = 944 MHz, is in red and blue while WISE 12 µm infrared image is in green. To present the structure of Raspberry, different colormaps and adjusted contrast levels were used. A linear scale is applied to all images. The inset is the ASKAP Stokes−V zoomed-in image showing the possible progenitor source. Credit: Lazarević et al., 2024.
Astronomers from the Western Sydney University in Australia and elsewhere report the detection of a new supernova remnant (SNR) candidate. The newfound SNR candidate, dubbed “Raspberry” due to its morphology, was identified in the near side of the Milky Way’s Scutum-Centaurus Arm. The findings were detailed in the Research Notes of the American Astronomical Society.
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