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With references to recent observational results on the nebula IC59, weapplied our previously developed Smoothed Particle Hydrodynamics (SPH) codewhich is based on Radiative Driven Implosion (RDI) model, to investigate thepossible formation mechanism for the observed morphological structures ofdifferently shaped BRCs. The simulation results confirmed the existence of the4th type morphology of BRCs -- type M BRC. We are able to find the necessarycondition for the appearance of the type M BRC based on the fact that thesimulated physical properties of the cloud are consistent with observations onIC59. More importantly, the prospect of RDI triggered star formation by RDImodel in all of the observed type M BRCs is ruthlessly eliminated.

An Investigation on the Morphological Structure of IC59: A New Type of Morphology of BRCs?