Guest: Novel Clues to the Formation of Ultra-Compact Dwarf Galaxies
In today’s bite, we look at some newly observed systems in the Virgo cluster. These observations provide clues to understanding how some of the most dense galaxies known to us form.
In today’s bite, we look at some newly observed systems in the Virgo cluster. These observations provide clues to understanding how some of the most dense galaxies known to us form.
Most gravitational-wave models throw away uncertainty, which could make Einstein’s theory look wrong when it isn’t. Today’s authors show when this could happen and how to take care of the problem.
Using low frequency radio observations of the galaxy NGC 2276 with the uGMRT and LOFAR telescopes, the authors discover that the galaxy has a trail of gas about 100 kiloparsecs long! As the galaxy moves through the local ionised medium, the pressure exerted on it removes gas from it’s disk.
Stars have spots that can mess with our planetary atmosphere observations. Using JWST, today’s authors take advantage of the unique TOI-3884 system to directly probe one of these regions.
The distribution of post-starburst regions within galaxies is linked to diverse quenching pathways that are likely driven by mergers. Guest author, Emmy Wisz, explains how different star formation histories could be the key to understanding quenching mechanisms.
Another day, another interesting LIGO-Virgo-KAGRA detection! Find out why the extreme parameters of GW231123 create problems for gravitational wave modelers and may have some new information about black hole formation!