In today’s paper: how does tidal dissipation and gravitational wave emission affect the result of encounters between stars and black hole binaries in stellar clusters?
Can machine learning and photometry help us uncover water on distant planets? Read on to find out!
Today’s paper puts simulation-based theories to the test as we look at some of the most massive disk galaxies and find out how they grew to their enormous sizes!
In today’s paper, the authors test the theory that the earliest, metal-poorest stars are the primary source of binary black hole mergers.
We’re always told not to judge a book by it’s cover, but what about galaxies? Today’s authors try to find out!
Today’s author gets out their umbrella to model planets that graze their stellar hosts.