A Software Solution for Tracking Down Gravitational Wave Sources
Researchers explore a new way to schedule observations in the hopes that we can make the most of limited telescope time when a new gravitational wave signal is detected.
Researchers explore a new way to schedule observations in the hopes that we can make the most of limited telescope time when a new gravitational wave signal is detected.
Were the first stars in the universe all massive, or did low-mass stars form in their midst? New research suggests that magnetic fields might have been the deciding factor.
The Milky Way hosts a large number of binary stars with equal masses and wide orbits. A new analysis of data from the Gaia spacecraft may help researchers understand how these systems formed.
What’s responsible for the arrangement of ultra-diffuse galaxy NGC5846-UDG1’s (many!) globular clusters?
What can the polarization of light around the core of Centaurus A tell us about the physics at play in such a high-energy environment?
In the Sun’s atmosphere, a massive eruption of plasma is brewing — how can we predict if a coronal mass ejection will cause a damaging geomagnetic storm?
Astronomers have tracked down a second millisecond pulsar in a nearby globular cluster. Can this discovery help us understand why these systems are so hard to find?
Researchers survey galaxies billions of years ago to understand how the Milky Way grew into the galaxy it is today.
Astronomers present evidence for a fourth circumplanetary disk candidate and, for the first time, an estimate of the mass of such a disk.
Researchers use fractal geometry for the first time to simulate realistic emission nebulae around hot young stars.