Ministers from the world’s leading industrialised nations agreed last
week to step up efforts to save science in Eastern Europe. But they stopped
short of creating a fund to pay for it.
The meeting of the OECD in Paris agreed to set up a new ‘forum’ to help
countries to make ‘intelligent choices’ on big science projects, such as
particle accelerators and research into the human genome. The ministers
asked the OECD to carry out a full inventory of all ‘big science’ facilities
in Eastern and Central Europe.
They pinpointed four ‘vital areas’ for cooperation with Eastern Europe:
training, strengthening the science infrastructure, technology transfer
and the conversion of military industry to civilian needs.
Russian science minister Boris Saltykov, who attended the meeting as
an observer, said that there had been ‘broad agreement’ on the idea of a
special fund or agency to support basic research in Eastern Europe. But
the form of the fund remains unclear.
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The French research minister, Hubert Curien, hinted that France will
soon take the initiative on the idea of an international agency to fund
science in the East. ‘The governments of interested countries must get together
now and it is not impossible that France may play a major role in coordinating
this business,’ he said.
Britain, Germany, Italy and the Netherlands backed the French idea.
But the US was less keen. Allan Bromley, science adviser to President Bush,
argued for joint initiatives and said that the US was looking for ways to
ensure that money ‘goes to science, not bureaucracy’ and only to ‘outstanding
scientists’.
Curien, who chaired the OECD meeting, warned that the new forum would
not be an excuse to wheel out ‘all the ideas which have been put on ice,
probably for good reasons’.
Bromley stressed that ‘science now needs such expensive instruments
that no country can go it alone’. This, together with the ending of the
Cold War, meant that ‘for the first time, we are dealing with the true internationalisation
of science’.
![Astronomers have long known that understanding how star clusters come to be is key to unlocking other secrets of galactic evolution. Stars form in clusters, created when clouds of gas collapse under gravity. As more and more stars are born in a collapsing cloud, strong stellar winds, harsh ultraviolet radiation and the supernova explosions of massive stars eventually disperse the cloud, and their light can bear down on other star-forming regions in the galaxy. This process is called stellar feedback, and it means that most of the gas in a galaxy never gets used for star formation. Researching how star clusters develop can answer questions about star formation at a galactic scale. Now, the state of the art has been further developed with both Hubble and Webb working together to provide a broad-spectrum view of thousands of young star clusters. An international team of astronomers has pored over images of four nearby galaxies from the FEAST observing programme (#1783), trying to solve this mystery. Their results show that it is the most massive star clusters that clear away their gaseous shroud the fastest, and begin lighting their galaxy the earliest. The team identified nearly 9000 star clusters in the four galaxies in different evolutionary stages: young clusters just starting to emerge from their natal clouds of gas, clusters that had partially dispersed the gas (both from Webb images), and fully unobstructed clusters visible in optical light (found in Hubble images). With Webb???s ability to peer inside the gas clouds, they were able to then estimate the mass and age of each cluster from its light spectrum. This image shows a section of one of the spiral arms of Messier 51 (M51), one of the four galaxies studied in this work, as seen by Webb???s Near-Infrared Camera (NIRCam). The thick clumps of star-forming gas are shown here in red and orange, representing infrared light emitted by ionised gas, dust grains, and complex molecules such as polycyclic aromatic hydrocarbons (PAHs). Within these gas complexes, each tens or hundreds of light years across, Webb reveals the dense, extremely bright clusters of massive stars that have just recently formed. The countless stars strewn across the arm of the galaxy, many of which would be invisible to our eyes behind layers of dust, are also laid bare in infrared light. [Image description: A large, long portion of one of the spiral arms in galaxy M51. Red-orange, clumpy filaments of gas and dust that stretch in a chain from left to right comprise the arm. Shining cyan bubbles light up parts of the gas clouds from within, and gaps expose bright star clusters in these bubbles as glowing white dots. The whole image is dotted with small stars. A faint blue glow around the arm colours the otherwise dark background.]](https://images.newscientist.com/wp-content/uploads/2026/05/13114322/SEI_296271016.jpg)


