VIIZw 403: a BCD with a noncoeval starburst
| dc.creator | Silich, S. | |
| dc.creator | Tenorio-Tagle, G. | |
| dc.creator | Munoz-Tunon, C. | |
| dc.creator | Cairos, L. M. | |
| dc.date | 2001-04-20 | |
| dc.date.accessioned | 2026-07-25T11:32:27Z | |
| dc.description | 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. | |
| dc.description | 1 page, 1 figure, Conference Proceedings: Ionized Gaseous Nebulae, to be published in Rev. Mex. A.A. Conf. Ser | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0104340 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0104340 | |
| dc.identifier.uri | https://dspace.dare.co.zw/handle/123456789/3561 | |
| dc.subject | Astrophysics | |
| dc.title | VIIZw 403: a BCD with a noncoeval starburst | |
| dc.type | text |