Most Population III Supernovae are Duds

dc.creatorKurucz, Robert L.
dc.date2008-08-25
dc.date.accessioned2026-07-07T09:58:13Z
dc.date.available2026-07-07T09:58:13Z
dc.descriptionOne Population III dud supernova produces enough oxygen to enable ten million solar masses of primordial gas to bind into M dwarfs. This is possible because radiation from other Population III stars implodes the mixture of oxygen ejecta and primordial gas into a globular cluster. Model atmosphere calculations for oxygen dwarfs show that water blocks most of the infrared flux. The flux is redistributed into the visible to produce an unfamiliar, distinctive energy distribution. One million dud supernovae in a large protogalaxy are sufficient to produce the "dark matter" halo.
dc.description4 pages, 7 figures
dc.identifierhttps://arxiv.org/abs/0808.3282
dc.identifierhttp://arxiv.org/abs/0808.3282
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/167637
dc.subjectAstrophysics
dc.titleMost Population III Supernovae are Duds
dc.typetext

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