VIIZw 403: a BCD with a noncoeval starburst
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The recent history of star formation in VIIZw 403 is analyzed taking into account the dynamics of the starburst blown superbubble and the restrictions that follow from X-ray observations, and from our H$α$ data. Our results show that the starburst energizing VIIZw 403 is NOT coeval, but rather the star forming phase has lasted for more than 30Myr and at such a low pace that most probably the newly processed metals will not be ejected into the intergalactic medium.
1 page, 1 figure, Conference Proceedings: Ionized Gaseous Nebulae, to be published in Rev. Mex. A.A. Conf. Ser
1 page, 1 figure, Conference Proceedings: Ionized Gaseous Nebulae, to be published in Rev. Mex. A.A. Conf. Ser