Mass-luminosity ratio in NGC 5236

Details Mass-luminosity ratio in NGC 5236 Mass-luminosity ratio in NGC 5236

Nov 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..73..193a&link_type=abstract

Astrophysics and Space Science, Volume 73, Issue 1, pp.193-197

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

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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