VIIZw 403: a BCD with a noncoeval starburst

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dc.creatorSilich, S.
dc.creatorTenorio-Tagle, G.
dc.creatorMunoz-Tunon, C.
dc.creatorCairos, L. M.
dc.date2001-04-20
dc.date.accessioned2026-07-07T01:58:16Z
dc.date.available2026-07-07T01:58:16Z
dc.descriptionThe 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.
dc.description1 page, 1 figure, Conference Proceedings: Ionized Gaseous Nebulae, to be published in Rev. Mex. A.A. Conf. Ser
dc.identifierhttps://arxiv.org/abs/astro-ph/0104340
dc.identifierhttp://arxiv.org/abs/astro-ph/0104340
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2702
dc.subjectAstrophysics
dc.titleVIIZw 403: a BCD with a noncoeval starburst
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