On the possible explosion in the Carina nebula

The consideration of the additional data on the distribution of OB stars, o f the dust matter (the IRAS data at 100 mu m, and of the results of observa tions 120-300 mu m), of the X-ray emission, of the continuum radio emission , and of the data on the proper motions of stars in the Carina nebula, prov ed the made suggestion (Tovmassian et al., 1993, 1994), that the observed s pecific distribution of the mentioned objects in the Carina nebula could be due to some explosion which took place in its central region.