Abstract
The mass-to-light ratio in NGC 5236 was studied in terms of four spheroids. The resulting values are quite small and increasing from the centre outwards, suggesting that Population I stars are rather uniformly distributed over its body with a certain concentration towards the central region.
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Agüero, E.L. Mass-luminosity ratio in NGC 5236. Astrophys Space Sci 73, 193–197 (1980). https://doi.org/10.1007/BF00642374
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DOI: https://doi.org/10.1007/BF00642374