One of the most important observations by the next generation of giant telescopes will be made by pointing towards the Supermassive Black Hole at the center of our galaxy.
In the latest of our #UndergradResearch series, discover how Anna Estes used ALMA to characterize Proxima Centauri’s flaring emissions at millimeter wavelengths!
How does the structure of the smallest galaxies vary with different environments? Today’s authors use the ELVES survey to investigate!
How big is a galaxy cluster? Today’s authors use the remnants of destroyed galaxies to define the edge of galaxy clusters.
What does the surface of a star look like? Today’s authors observe ζ And using long-baseline interferometry to find out!
Today’s authors work out a full orbital solution for a binary microlensing system, indicating the method’s potential to probe the mass distribution of dark objects.