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- W2051289353 abstract "view Abstract Citations (322) References (102) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Cosmological consequences of Population III stars Carr, B. J. ; Bond, J. R. ; Arnett, W. D. Abstract The possible cosmological consequences of Population III stars are examined. Their dark remnants could provide the 'missing mass'. Their light could have produced either the entire 3 K background or observable distortions in its spectrum. Their heat or explosions could have reionized the universe and perhaps produced galaxies. Their helium yield could suffice to provide an alternative explanation for the observed 'primordial' abundance, and their heavy-element yield could have produced a burst of pregalactic enrichment. It is discussed which sort of stars could best fulfill these roles and conclude that the most plausible candidates would be 'Very Massive Objects' in the mass range 100-100,000 solar masses. Even if Population III stars played none of these roles, consideration of the associated effects places strong constraints on their mass spectrum and formation epoch. Publication: The Astrophysical Journal Pub Date: February 1984 DOI: 10.1086/161713 Bibcode: 1984ApJ...277..445C Keywords: Cosmology; Star Distribution; Stellar Mass; Supermassive Stars; Black Holes (Astronomy); Main Sequence Stars; Mass Spectra; Mass To Light Ratios; Missing Mass (Astrophysics); Nuclear Fusion; Radiation Effects; Red Shift; Stellar Evolution; Stellar Radiation; Stellar Spectra; Astrophysics full text sources ADS |" @default.
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- W2051289353 title "Cosmological consequences of Population III stars" @default.
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