Statistics for MUSE observations of the giant low surface brightness galaxy Malin 1: Numerous HII regions, star formation rate, metallicity, and dust attenuation
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MUSE observations of the giant low surface brightness galaxy Malin 1: Numerous HII regions, star formation rate, metallicity, and dust attenuation | 0 |
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January 2025 | 0 |
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MUSE observations of the giant low surface brightness galaxy.pdf | 13 |