Scientists have discovered the first gamma-ray eclipses from a special type of binary star system using data from NASA’s Fermi Gamma-ray Space Telescope.
These so-called spider systems each contain a pulsar and rapidly rotating remains of a star that exploded in a supernova – that slowly erodes its companion.
Spider systems develop because one star in a binary evolves more swiftly than its partner.
A binary system is one in which two stars orbit around a common centre of mass, that is they are gravitationally bound to each other.
Pulsars are rapidly spinning neutron stars.
They are extremely dense stars composed almost entirely of neutrons and having a diameter of only 20 km (12 miles) or less.
They emit concentrated streams of radiation far across the space.