
How to Make “A Star that Should Not Exist”
The low-mass primitive halo star, SDSS J102915+172927, puzzled astronomers because of it’s extremely low metal content. This article aims to answer under what physical conditions can a star like this form.
The low-mass primitive halo star, SDSS J102915+172927, puzzled astronomers because of it’s extremely low metal content. This article aims to answer under what physical conditions can a star like this form.
Could stars with masses 100,000 times more massive than our Sun exist? Are these the possible progenitors for supermassive black holes that litter our universe today?
In this article the authors simulate the collapse of a magnetized, turbulent molecular cloud core to see if rotationally supported discs can form around central protostars.
Could higher than expected mass-loss rates for evolved massive stars lead to progenitors for peculiar Supernovae?
Could the interaction of the pre-solar core with a nearby supernova trigger the formation of our Solar System?