HD molecules at high redshift A low astration factor of deuterium in a solar-metallicity DLA system at z=2.418

Noterdaeme P.; Petitjean P.; Ledoux, C; Srianand R.; Ivanchik, A.

Abstract

We present the detection of deuterated molecular hydrogen (HD) in the remote Universe in a damped Lyman-α cloud at Zabs toward the quasar SDSS J143912.04+111740.5. This is a unique system in which H2 and CO molecules are also detected. The chemical enrichment of this gas derived from Zn II and S II is as high as in the Sun. We measure N(HD)/2N(H 2),= 1.5-0.4 1.5+0.6 × 10-5, which is significantly higher than the same ratio measured in the Galaxy and close to the primordial D/H ratio estimated from the WMAP constraint on the baryonic matter density (Ωb). This indicates a low astration factor of deuterium that contrasts with the unusually high chemical enrichment of the gas. This can be interpreted as the consequence of an intense infall of primordial gas onto the associated galaxy. Detection of HD molecules at high-z also opens the possibility of obtaining an independent constraint on the cosmological-time variability of μ, the proton-to-electron mass ratio. © 2008 ESO.

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Título según WOS: HD molecules at high redshift A low astration factor of deuterium in a solar-metallicity DLA system at z=2.418
Título según SCOPUS: HD molecules at high redshift a low astration factor of deuterium in a solar-metallicity DLA system at z = 2.418
Título de la Revista: ASTRONOMY & ASTROPHYSICS
Volumen: 491
Número: 2
Editorial: EDP SCIENCES S A
Fecha de publicación: 2008
Página de inicio: 397
Página final: 400
Idioma: English
URL: http://www.aanda.org/10.1051/0004-6361:200810414
DOI:

10.1051/0004-6361:200810414

Notas: ISI, SCOPUS