Richard Mushotzky

About 25,000 light-years from Earth, in the constellation Sagittarius, a dense veil wraps around the neutron star GX 13+1. It scatters X-ray photons the way fog scatters streetlight, and for a long time it hid the source's true power from astronomers.

The galaxy MCG+11-11-032 is relatively close to us: its light takes about 150 million years to reach us. At its center, like in most large galaxies, sits a supermassive black hole. But a few years ago, astronomers began to suspect: what if there are two? The clue came from the X-ray spectrum.

The Perseus galaxy cluster is a giant metropolis of thousands of star islands, bathed in an invisible ocean of scorching gas. Like urban smog, this gas preserves traces of all the chemical factories that have operated in galaxies for billions of years: supernova explosions that scatter freshly forged atoms across the surroundings.

An orchestra of hundreds of galaxies performs a symphony in X-rays, but until recently we heard only a general hum. The Coma Cluster is about a thousand galaxies immersed in a cloud of scorching gas at a temperature of one hundred million degrees. This gas glows in X-rays, and its spectrum tells us how it moves.