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The first science ever with APEX

13.07.2006
This week, Astronomy & Astrophysics is publishing a series of 26 articles dedicated to the first science done with the APEX telescope. The APEX telescope is located at 5100 metres, at Chajnantor in the Atacama Desert (northern Chile). It will be dedicated to observing the sky of the Southern hemisphere at “sub-millimetre wavelengths”. It covers so-called “atmospheric windows” – the wavelengths at which the Earth’s atmosphere is partially transparent – between 0.1 mm and 1 mm. APEX will thus be observing the “cold universe”, which radiates at these wavelengths.

This “cold universe” includes the cold clouds where young stars are presently forming, and in which the temperature is only -260°C. We believe our solar system formed from one of these cold clouds. Astronomers studying these clouds are trying to understand what our solar system may have looked like just prior to and just after the birth of the Sun. Other applications for APEX will be the study of stars losing mass in the last stages of their evolution and of star-forming regions in different galaxies.

One scientific highlight in this issue is the discovery of a new interstellar molecule CF+, using both APEX and the IRAM 30-metre telescope near Granada in Spain. Prior to this discovery, there was only one fluorine-containing molecular species found in space so far. This molecule was found in the neutral gas region adjoining the Orion Nebula.

Another premiere is the detection – again in the Orion region – of radiation from carbon monoxide (CO) at a wavelength of 0.2 mm. This is the work of Martina Wiedner (University of Cologne, Germany) and her colleagues. These wavelengths are very difficult to investigate, both because the water vapour in the atmosphere attenuates the signal, and because the light-collecting system technology is less advanced at these wavelengths. The detection of CO at these wavelengths proves the efficiency of APEX, and later that of ALMA.

Finally, H2D+ radiation was detected from several clouds in the Southern hemisphere by two different teams: one lead by Jorma Harju (University of Helsinki, Finland), the other with Michiel Hogerheijde (Leiden Observatory, Netherlands) and collaborators. The H2D+ ion is interesting because it traces gas that is so cold (a few degrees above the absolute zero) that only the lightest molecular species, including H2D+, have not frozen out onto the surfaces of dust grains.

Along with the Japanese 10-m ASTE telescope, APEX is the first telescope dedicated to the sub-millimetre wavelengths in the Southern hemisphere. Until now, this sort of science was only carried out in the Northern hemisphere. APEX is indeed a forerunner to a large array of sub-millimetre telescopes (ALMA or Atacama Large Millimeter Array). ALMA will be built on the Chanjantor site, by a consortium from the United States, Europe, and Japan. ALMA will consist of 50 telescopes of the same dimensions (12-m diameter) as APEX, in an array which will extend over 10 km. It will be built on the Chajnantor site between 2003 and 2012. APEX itself was constructed by a consortium of the Max-Planck-Institut für Radioastronomie (Bonn, Germany), ESO, and the Onsala Space Observatory (Sweden). Apart from its relevance in the course of the ALMA project, APEX is interesting in its own right, as illustrated by the wealth of results published in this special issue.

Jennifer Martin | alfa
Further information:
http://www.edpsciences.org
http://www.edpsciences.org/articles/aa/abs/2006/29/contents/contents.html

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