NGC 4736 (UGC 7996, 1248+4123) -- This ringed Sab galaxy has many peculiar features, suggesting it is in the final stages of a merger. It is one of the UV-bright LINERs studied in more detail by Maoz et al. (1995), and has two bright unresolved UV point sources, one on the nucleus and one $2.5" to the north. Using the algorithm of Maoz et al. (1996), we measure for the nuclear point source a UV flux density f![]() ![]() |
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