
doi: 10.1086/186214
In this Letter we present the detection, for the first time, of double-peaked broad Balmer Hα and Hβ emission-line profiles in a luminous IRAS galaxy : IRAS 02366-3101 with log L FIR =10.94 L ⊙ . This detection shows that IRAS 02366-3101 is a candidate to host an accretion disk around a supermassive black hole in its nucleus, although other alternatives cannot be ruled out
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