Making Supermassive Black Holes Spin
Where does the angular momentum come from that causes supermassive black holes to spin on their axes and launch powerful jets?
Where does the angular momentum come from that causes supermassive black holes to spin on their axes and launch powerful jets?
Our measurements of exoplanet atmospheres may be influenced by the activity of the planets’ host stars.
Are small satellite galaxies usually distributed evenly around their larger galactic hosts? Evidence suggests otherwise.
Astrobites explores the role of magnetic fields in X-ray emission from the centers of active galaxies.
What can we learn about a coronal mass ejection as it passes between us and a distant pulsar?
Have you been contributing your computer idle time to the Einstein@Home project? If so, you’re partly responsible for the program’s recent discovery of a new double-neutron-star system!
The Milky Way’s dense central bulge is a very different environment than the galactic disk. Do the differences affect the ability of planets to form there?
Astrobites reports on a closer look at the Sun’s past activity levels.
A major challenge for modern supernova surveys is identifying the galaxy that hosted each explosion. Is there an accurate and efficient way to do this that avoids investing significant human resources?
What impact did X-rays from the first binary star systems have on the universe around them? A new study suggests this radiation may have played an important role during the reionization of our universe.
Astrobites tackles the question of where blue straggler stars come from — as well as where they’re going.
These images of comet 67P mark the first time we’ve been able to study the inner coma of a comet at this level of detail.