2003ApJ...589...53H


Query : 2003ApJ...589...53H

2003ApJ...589...53H - Astrophys. J., 589, 53-57 (2003/May-3)

Chemical composition of the early universe.

HARWIT M. and SPAANS M.

Abstract (from CDS):

A prediction of standard inflationary cosmology is that the elemental composition of the medium out of which the earliest stars and galaxies condensed consisted primarily of hydrogen and helium 4He, with small admixtures of deuterium, lithium 7Li, and 3He. The most redshifted quasars, galaxies, and Lyα absorbers currently observed, however, all exhibit at least some admixture of heavier elements, as do the most ancient stars in the Galaxy. Here we examine ways in which the abundance of these same elements, if present before the epoch of Population III formation, might be observationally established or ruled out.

Abstract Copyright: ∼

Journal keyword(s): Cosmology: Miscellaneous - Cosmology: Early Universe - Nuclear Reactions, Nucleosynthesis, Abundances

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SDSS J104433.04-012502.0 QSO 10 44 33.040 -01 25 02.08     21.81     ~ 182 1
2 QSO B1422+2309 BLL 14 24 38.0938 +22 56 00.587   16.77 15.84 14.79   ~ 464 1
3 [PBW92] 1422+231 gLS 14 24 38.09400 +22 56 00.5900   16.77 15.84 14.79   ~ 359 0

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