First optical spectroscopy of SNR G25.1-2.3 reveals shock-heated gas with varying electron densities, filamentary structures, and a new HI hole consistent with the remnant's size.
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Optical observations and atomic environment of supernova remnant G25.1-2.3
First optical spectroscopy of SNR G25.1-2.3 reveals shock-heated gas with varying electron densities, filamentary structures, and a new HI hole consistent with the remnant's size.