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- W2000594528 abstract "Observations of the distribution of neutral hydrogen around the supernova remnants G 5.3 - 1.1 and G 24.7 + 0.6 made with the radio telescope RATAN-600 with resolution 2' x 130' x 6.3 kmsec have shown that these shells are surrounded by expanding H I shells of diameter 68 and 128 pc with masses 640 and 4.6 x 10/sup 3/ M/sub sun. The most probable mechanism of their formation is the outflow of a stellar wind during the lifetime of the stars on the main sequence. The masses of the stars have been estimated (17 and 38 M//sub sun/), and also the mass of the gas ejected in the supernova explosions" @default.
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- W2000594528 date "1987-01-01" @default.
- W2000594528 modified "2023-09-27" @default.
- W2000594528 title "Neutral hydrogen around some young supernova remnants" @default.
- W2000594528 cites W2058314850 @default.
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- W2000594528 doi "https://doi.org/10.1007/bf01005396" @default.
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