EDP Sciences
Free access
Volume 491, Number 2, November IV 2008
Page(s) 397 - 400
Section Cosmology (including clusters of galaxies)
DOI http://dx.doi.org/10.1051/0004-6361:200810414
Published online 01 October 2008

A&A 491, 397-400 (2008)
DOI: 10.1051/0004-6361:200810414

HD molecules at high redshift

A low astration factor of deuterium in a solar-metallicity DLA system at z = 2.418
P. Noterdaeme1, P. Petitjean1, C. Ledoux2, R. Srianand3, and A. Ivanchik4

1  Institut d'Astrophysique de Paris, CNRS - Université Pierre et Marie Curie, 98bis Bd Arago, 75014 Paris, France
    e-mail: [noterdaeme;petitjean]@iap.fr
2  European Southern Observatory, Alonso de Córdova 3107, Casilla 19001, Vitacura, Santiago 19, Chile
    e-mail: cledoux@eso.org
3  Inter University Centre for Astronomy and Astrophysics, Post Bag 4, Ganesh Khind, Pune 411 007, India
    e-mail: anand@iucaa.ernet.in
4  Ioffe Physical Technical Institute, St Petersburg 194021, Russia
    e-mail: iav@astro.ioffe.ru

Received 18 June 2008 / Accepted 20 September 2008

We present the detection of deuterated molecular hydrogen (HD) in the remote Universe in a damped Lyman-$\alpha$ cloud at $z_{\rm abs}=2.418$ 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 $N({\rm HD})/2 N({\rm H_2})=1.5^{+0.6}_{-0.4} \times 10^{-5}$, 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 ( $\Omega_{\rm b}$). 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 $\mu$, the proton-to-electron mass ratio.

Key words: cosmology: observations -- galaxies: high-redshift -- galaxies: ISM -- quasars: absorption lines -- quasars: individual: SDSS J143912.04+111740.5

© ESO 2008

What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access.

An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.

  • If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
  • You can define your own OpenURL resolver with your EDPS Account.
    In this case your choice will be given priority over that of your library.
  • You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.