NASA discovers first gamma-ray eclipses from Spider star systems

Data from NASA’s Fermi Gamma-ray Space Telescope has been used to discover the first gamma-ray eclipses from a special type of binary star system. Check details here.

NASA discovers first gamma-ray eclipses from a special type of binary star system. (NASA/Sonoma State University, Aurore Simonnet)

Every one is aware of the Solar and Lunar eclipses, but there is something called gamma-ray eclipses too. Data from NASA's Fermi Gamma-ray Space Telescope has been used by scientists to discover the first gamma-ray eclipses from a special type of binary star system. These so-called spider systems contain a pulsar – the superdense, rapidly rotating remains of a star that exploded in a supernova – that slowly erodes its companion, NASA informed.

"An international team of scientists scoured over a decade of Fermi observations to find seven spiders that undergo these eclipses, which occur when the low-mass companion star passes in front of the pulsar from our point of view. The data allowed them to calculate how the systems tilt relative to our line of sight and other information," the space research organisation said in a report.

Spider systems develop because one star in a binary evolves more swiftly than its partner. When the more massive star goes supernova, it leaves behind a pulsar. This stellar remnant emits beams of multiwavelength light, including gamma rays, that sweep in and out of our view, creating pulses so regular they rival the precision of atomic clocks.

Early on, a spider pulsar feeds off its companion by siphoning away a stream of gas. As the system evolves, the feeding stops as the pulsar begins to spin more rapidly, generating particle outflows and radiation that superheat the companion's facing side and erode it.

Scientists divide spider systems into two types named after spider species whose females sometimes eat their smaller mates. Black widows contain companions with less than 5 percent of the Sun's mass. Redback systems host bigger companions, both in size and mass, weighing between 10 percent and 50 percent of the Sun.

Researchers can calculate the masses of spider systems by measuring their orbital motions. Visible light observations can measure how quickly the companion is traveling, while radio measurements reveal the pulsar's speed. However, these rely on motion towards and away from us. For a nearly face-on system, such changes are slight and potentially confusing. The same signals also could be produced by a smaller, slower-orbiting system that's seen from the side. Knowing the system's tilt relative to our line of sight is vital for measuring mass.

The tilt's angle is normally measured using visible light, but these measurements come with some potential complications. As the companion orbits the pulsar, its superheated side comes in and out of view, creating a fluctuation in visible light that depends on the tilt. However, astronomers are still learning about the superheating process, and models with different heating patterns sometimes predict different pulsar masses.

Gamma rays, however, are only generated by the pulsar and have so much energy that they travel in a straight line, unaffected by debris, unless blocked by the companion. If gamma rays disappear from the data set of a spider system, scientists can infer that the companion eclipsed the pulsar. From there, they can calculate the system's tilt into our sight line, the stars' velocities, and the pulsar's mass.