Ripples in Time: The Transient Nature of Mysterious M Stars
Today’s authors, kick back, relax, and try to understand how some mysterious M dwarfs change over time.
Finger on the Pulse of Magnetic Fields on delta Scuti and gamma Dor Variables
The oscillation modes of stars can tell us about their interior structure. However, strong magnetic fields can damp out these modes and make them undetectable. These authors look at two types of stars with oscillations to see what their magnetic fields are like.
Shock(ing) Emission from a Young Sun
There’s always more to learn about epsilon Eridani– the nearest sun-like star that hosts an exoplanet. These authors work to determine the emission processes and physics associated with radio emission detected from epsilon Eridani in 2020.
Today in (Astro) Shop Class: How to build a molecular cloud?
The authors of today’s paper create a model of molecular clouds that can help us understand how they form stars!
Can you tell if a star got too close to a black hole?
The authors of today’s paper study emission lines in a spectrum to determine if they are caused by a star falling into a black hole!
The Cosmic Tale of Star Birth
In today’s astrobite, find out how stars and clusters are formed by looking at their size and age.