Berlin
GERMAN scientists are demanding a crash programme to strengthen the
country’s defences against infectious diseases. The country’s famed efficiency
in record keeping, they say, is almost entirely absent when it comes to
monitoring diseases such as hepatitis, salmonella poisoning and even measles.
Immunisation programmes have been neglected, data on the frequency of infectious
outbreaks are unreliable or nonexistent and when local outbreaks occur often
little effort is made to track down their source.
Later this year, the German government plans to introduce a law that will
require doctors to report all cases of infectious disease. A draft of the
proposed law will be released for public comment next month. Yet according to
Rüdiger Fock, head of infectious disease epidemiology at the Robert Koch
Institute in Berlin, this law is only a small part of what is needed.
Fock claims that German doctors currently report only about 10 per cent of
hepatitis cases, for instance, because they realise that their information is
vanishing into a “black hole”. In contrast, they voluntarily report almost all
AIDS cases because they know these reports are closely watched by the
government.
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Fock warns that some of the neglected diseases pose a real threat. For
example, only about 30 per cent of the German population are adequately
immunised against diphtheria. With people streaming back and forth between
Germany and the former Soviet Union, where diphtheria has reached epidemic
levels, Fock says he would not be surprised if the disease soon takes hold in
Germany. What is needed, he says, is a revival of epidemiology, which has all
but died out in Germany.
To promote this message, the Robert Koch Institute has begun to emulate the
American Centers for Disease Control and Prevention (CDC). Last year it began
publishing a weekly bulletin, which is modelled on the CDC’s Morbidity and
Mortality Weekly Report. Lyle Peterson, an epidemiologist from the CDC, has
been based permanently in Berlin since last year. Other CDC scientists travel
regularly to Germany to conduct short training sessions for local health
officials.
Within the past year, Peterson has led investigative teams to regions of
Germany where there have been outbreaks of Escherichia coli O157 and
salmonella poisoning. Those were the first such investigations in Germany since
the Second World War, says Peterson.
Some German scientists blame the country’s poor epidemiology on its strict
data protection laws, which prohibit local health authorities and doctors from
disclosing to researchers the identities or other personal details of patients.
But Ulrich Keil, a leading epidemiologist at the University of Münster,
says these difficulties can be overcome with a bit of persistence. The problem
is not so much the law, he claims, as “laziness”.
![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)


