Kinematics of the Interstellar Medium in the Galaxy IC10

Physics

Scientific paper

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Scientific paper

The BCD-galaxy IC10 possesses a very large number of Wolf-Rayet stars and contains a large nonthermal superbubble (size > 250 pc). We present the kinematic analysis of the ionized and neutral gas near WR-stars and in the region of the superbubble using the Fabry-Perot H-alpha-line observations performed with 6-m SAO RAS telescope and VLA 21-cm radio observations. The results of the analysis are discussed.

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