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We report on the investigation of three young stellar objects in the rarely studied dark cloud L1188. Using near- to far-infrared (2MASS, MSX, IRAS and ISO) data we derived their spectral energy distributions which allowed an approximate determination of their evolutionary stages. Two objects were classified as Class I protostars and one source was found to be a Class 0 candidate in the earliest phase of stellar evolution.

Related paper:

Title: Young Stellar Objects in L1188

Authors: Könyves, V.; Moór, A.; Kiss, Cs.; Ábrahám, P.

Journal: Baltic Astronomy, Vol. 13, p. 470-473 (2004)