A white dwarf and a red dwarf star have been discovered closely orbiting each other emitting radio pulses every two hours. Their findings means we know it isn't just neutron stars that emit such ...
"The goal of this project was to explore the fundamental low-mass limit of the star and brown dwarf formation process." ...
One member of the system is an M dwarf, also known as a red dwarf, a small, low-mass star found in abundance throughout the galaxy. The other member appears to be a white dwarf, or the leftover ...