Astronomers, using the unique capabilities offered by the high-resolution spectrograph UVES on ESO's Very Large Telescope, have found a metal-rich hydrogen cloud in the distant universe. The result may help to solve the missing metal problem and provides insight on how galaxies form.
"Our discovery shows that significant quantities of metals are to be found in very remote galaxies that are too faint to be directly seen", said Celine Peroux (ESO), lead-author of the paper presenting the results .
The astronomers studied the light emitted by a quasar located 9 billion light-years away that is partially absorbed by an otherwise invisible galaxy sitting 6.3 billion light-years away along the line of sight.
The analysis of the spectrum shows that this galaxy has four times more metals than the Sun. This is the first time one finds such a large amount of 'metals'  in a very distant object. The observations also indicate that the galaxy must be very dusty.
Almost all of the elements present in the Universe were formed in stars, which themselves are members of galaxies. By estimating how many stars formed over the history of the Universe, it is possible to estimate how much metals should have been produced. This apparently straightforward reasoning has however since several years been confronted with an apparent contradiction: adding up the amount of metals observable today in distant astronomical objects falls short of the predicted value. When the contribution of galaxies now observed at cosmological distances is added to that of the intergalactic medium, the total amounts for no more than a tenth of the metals expected.
Studying distant galaxies is however a difficult task. The further a galaxy, the fainter it is, and the small or intrinsically faint ones won't be observed. This may introduce severe biases in the observations as only the largest and most active galaxies are picked up.
Astronomers therefore came up with other ways to study distant galaxies: they use quasars, most probably the brightest distant objects known, as beacons in the Universe.
Interstellar clouds of gas in galaxies, located between the quasars and us on the same line of sight, absorb parts of the light emitted by the quasars. The resulting spectrum consequently presents dark 'valleys' that can be attributed to well-known elements. Thus, astronomers can measure the amount of metals present in these galaxies – that are in effect invisible - at various epochs.
"This can best be done by high-resolution spectrographs on the largest telescopes, such as the Ultra-violet and Visible Echelle Spectrograph (UVES) on ESO's Kueyen 8.2-m telescope at the Paranal Observatory," said Péroux.
Her team studied in detail the spectrum of the quasar SDSS J1323-0021 that shows clear indications of absorption by a cloud of hydrogen and metals located between the quasar and us. From a careful analysis of the spectrum, the astronomers found this 'system' to be four times richer in zinc than the Sun. Other metals such as iron appear to have condensed into dust grains.
"If a large number of such 'invisible' galaxies with high metal content were to be discovered, they might well alleviate considerably the missing metals problem", said Péroux.
The full text of this release along with an image is available at http://www.eso.org/outreach/press-rel/pr-2006/pr-06-06.html
 The discovery is to appear in a paper published by Astronomy and Astrophysics ("The Most Metal-Rich Intervening Quasar Absorber Known", by C. Péroux et al.) and available in PDF format at http://www.edpsciences.org/articles/aa/pdf/press-releases/PRAA200602.pdf
The team is composed of Céline Péroux (ESO), Varsha Kulkarni and Joe Meiring (University of South Carolina, Columbia, USA), Roger Ferlet (Institut d'Astrophysique de Paris, France), Pushpa Khare (Utkal University, India), Jim Lauroesch (Northwestern University, Evanston, USA), Giovanni Vladilo (Osservatorio di Trieste, Italy), and Don York (University of Chicago, USA).
 For astronomers, metals are all chemical elements heavier than helium. The Sun, for example, is made mostly of hydrogen (73%) and helium (25%), and only 2% of 'metals'.
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