The authors of today’s paper seek to uncover what is occulted in the final moments of a massive star’s death. To this end, they outline the feasibility of measuring the background flux of “relic neutrinos” and connect them to their origins.
“But the stars that marked our starting fall away. We must go deeper into greater pain…” -Dante’s Inferno… and AGN, apparently
In today’s post, we interviewed Dr. Ann-Marie Madigan, an Assistant Professor at CU Boulder about her accomplishments & her journey in astronomy.
We report on Day 3 of the 2022 April APS Meeting!
We report on Day 2 of the 2022 April APS Meeting!
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?