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4U 2206+54 is one of the most intriguing X-Ray binaries. While showing properties closer to those of wind-fed supergiant X-Ray binaries, its optical co unterpart lies in the main sequence, and recently it has been suggested that it may harbor an accre tion disk (Finger et al. 2010). Only recently the real nature of the compact object has been r vealed by the discovery of X-Ray pulsations (Reig et al. 2009). A detailed analysis of ISGRI d ata on this source is shown. The pulse period of 4U 2206+54 is analyzed and the properties of i t pulse profile are discussed.

The role of ISGRI data on the discovery of pulsations in 4U 2206+54