Attacking the (Multi-)Messenger: Simulating a Kilonova
Neutron stars (NSs) are the most extreme objects known, composed of a form of matter so extraordinarily dense that it teeters on the brink of collapse into a black hole.
Neutron stars (NSs) are the most extreme objects known, composed of a form of matter so extraordinarily dense that it teeters on the brink of collapse into a black hole.
Everyone wants to find a habitable planet. The authors of today’s paper make a compelling case that the HR 5183 system is not the best place to look.
Pulsar timing arrays could localise individual sources of gravitational waves to host galaxies. The problem is, it’s so computationally difficult! This paper shows us a faster way.
Today’s paper looks at the impact of AGN feedback on X-ray emission around an unprecedented sample of galaxy groups!
The spectroscopists don’t want you to know that exoplanet atmospheres are actually three-dimensional! Today’s authors use computational climate models to study how we might be able to directly observe different planetary heating processes.
We interviewed Prof. Eve Lee of McGill University to learn all about planet and star formation ahead of her plenary talk at #AAS243!