On the possible explosion in the Carina nebula

The consideration of the additional data on the distribution of OB stars, of the dust matter (the IRAS data at 100 mu m, and of the results of observations 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, proved the made suggestion (Tovmassian et al., 1993, 1994), that the observed specific distribution of the mentioned objects in the Carina nebula could be due to some explosion which took place in its central region.