SIMBAD references

1999A&A...349L..13M - Astronomy and Astrophysics, volume 349L13-16 (1999/9-1)

Low deuterium abundance in the zabs=3.514 absorber towards APM 08279+5255.

MOLARO P., BONIFACIO P., CENTURION M. and VLADILO G.

Abstract (from CDS):

A high-resolution, high signal-to-noise HIRES-Keck spectrum of APM 08279+5255 reveals a feature in the HI Lyα profile of the zabs=3.514 absorber at the expected position of the corresponding DI Lyα line. The absorber shows a relatively simple velocity structure, with a major component detected in several metallic lines including CII, CIV, SiII, SiIII and Si IV. Modeling of the hydrogen column density with the minimum number of components yields (D)/(H)≃1.5x10–5. However, a more complex structure for the hydrogen cloud with somewhat ad hoc components would allow a higher (D)/(H). The system has a very low metallicity with [Si/H]≃-3.5 and [C/H]≃-4.0 and is therefore representative of essentially unprocessed material, with a deuterium abundance close to the primordial value. The present analysis favours the low D/H value of (D)/(H)=3.39±0.25x10–5 measured towards QSO 1009+2956 and QSO 1937-1009 (Burles & Tytler, ApJ...499..699B, 1998ApJ...507..732B) as the fiducial value of deuterium at high redshift.

Abstract Copyright: ∼

Journal keyword(s): cosmology: observations - cosmology: early Universe - galaxies: quasars: individual: APM 08279+5255 - nuclear reactions, nucleosynthesis, abundances

CDS comments: p. L15 : Q0014-813 misprint for 0014+813

Simbad objects: 6

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