THE PAST few years have seen the discovery of an entirely new kind of beast
living right here in our Galaxy. These objects flicker wildly, sometimes shining
so brightly that they are the most brilliant source of X-rays in the sky. The
radiation they give off shows that within them, matter and antimatter are
colliding. And they emit jets of electrons that appear to be speeding outwards
faster than light. Welcome to the world of the microquasar.
In many ways, microquasars mimic their big cousins, quasars. Quasars proper
are the brightest things in the Universe. They look like brilliant blue stars,
and emit colossal jets of electrons that stretch out into space for millions of
light years. The current theory is that at the heart of every quasar is a black
hole heavier than 10 million Suns. As gas from the surrounding galaxy falls
inwards, it forms a hot disc that swirls around the hole in grand slow motion.
But this is still a crude picture. One of the puzzles we have still to unravel
is why quasars emit those vast jets.
In human terms, quasars are not only very big, they’re very slow. A lifetime
is too short see a full-size quasar chewing up stars and spitting them out
again. So microquasars aren’t just interesting in their own right. A microquasar
does all the exciting things a quasar does—but it’s a million times
smaller and a million times faster.
The first microquasar was tracked down because astronomers thought it was a
real quasar. Somewhere near the heart of the Milky Way is an object emitting
gamma rays with…
![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)


