Using eROSITA to look at Beautiful AGN Blow-outs
In today’s paper, the authors use eROSITA to assemble a sample of the beautiful blow-outs that can occur in galaxies when AGN turn on.
In today’s paper, the authors use eROSITA to assemble a sample of the beautiful blow-outs that can occur in galaxies when AGN turn on.
Even though the Sun is the nearest star to us, there’s a lot we still don’t understand about it and its activity. These authors present an interesting case of a unique type of solar radio emission occurring under conditions it doesn’t normally do so.
Today we interview x-ray astronomer and professor at the University of Maryland, Dr. Richard Mushotzky, for his plenary talk at #AAS241!
We’ve updated and expanded our “Guide to the Electromagnetic Spectrum”! Read on to learn about all the different flavors of light in the Universe, where this light comes from, and how we can detect it.
For the first time, astronomers have detected the hot, diffuse circumgalactic medium — a perfect testbed for models of galactic feedback. So, how do our current models stack up against the new data?
M dwarfs are known to be really active when they’re young, which is bad for habitability. But what about old M dwarfs?