There’s a cluster of stars near the Milky Way’s center whose distribution and age puzzles scientists. Could an intermediate-mass black hole be the light that reveals the mystery?
In today’s paper: the sensitivity and power of JWST has allowed scientists to discover signs of at least two, if not three, unknown companions to NGC 3132’s central star!
In today’s paper, the authors analyze millimeter and submillimeter ALMA observations of a protoplanetary disk, and find kinematic signs of candidate companions within!
In today’s paper, the authors take another look at the HD 45354 planetary system, and come to new conclusions about the orbit of the two gas giants within!
The authors of today’s article argue that stripped B-type stars could be a source of false positives in the search for quiet, stellar-mass black holes in the Milky Way