Many assumptions are used as input for photoionization codes that model HII regions. Today’s paper explores how these assumptions are oversimplified and emphasizes the need for more physically realistic ones.
If every pulsar had more motion
Across the galactic plane
Then they’d all be surfin’
On fuzzy dark matter, yeah
What happens when supernova remnants interact with the surrounding environment? The authors of today’s paper use the X-rays from RCW 86 to try and find out!
M dwarf stars host single planet systems (only child) and multi-planet systems (siblings). Let’s explore the differences!
How do distant supermassive black holes affect their host galaxies? And how were they formed? Today’s paper explores these questions with a sample distant SMBHs discovered by JWST!
Did a galaxy ever lie to you? Likely not. But they can be crooked on a whole other level. In today’s bite, find out how the authors found a way to exploit the galaxy’s skewness to their advantage.