The Rapid Burster
These four images show an artist's impression of gas accreting onto the neutron star in the binary system MXB 1730-335, also known as the "Rapid Burster."
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Scientists observing a neutron star in the "Rapid Burster" system may have solved a 40-year-old mystery surrounding its puzzling X-ray bursts.

Discovered in the 1970s, the Rapid Burster is a binary system comprising a low-mass star in its prime and a neutron star -- the compact remnant of a massive star's demise. The gravitational pull of the neutron star strips its companion of some of its gas, which then forms an accretion disk and spirals toward the neutron star.

Most neutron star binary systems continuously release large amounts of X-rays, punctuated by additional X-ray flashes every few hours or days. But scientists have wondered for decades about what accounts for the Rapid Burster's sudden, erratic and extremely intense X-ray emissions -- a phenomenon seen only in one other binary system.

In the new study, researchers discovered that the neutron star's magnetic field creates a gap between the star and the disk around it, largely preventing it from feeding on matter from its stellar companion. Gas builds up until, under certain conditions, it hits the neutron star all at once, producing intense flashes of X-rays.

The new results provide the first evidence for what causes these so-called "type-II" bursts. The discovery was made with the European Space Agency's XMM-Newton mission and NASA's NuSTAR (Nuclear Spectroscopic Telescope Array) and Swift missions.

Full ESA story

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Elizabeth Landau 818-354-6425
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Jakob van den Eijnden +31-6-4816-3504
Anton Pannekoek Institute for Astronomy, University of Amsterdam, The Netherlands

Nathalie Degenaar/Anton Pannekoek +31-20-525-3994
Institute for Astronomy, University of Amsterdam, The Netherlands

Norbert Schartel +34-91-8131-184
European Space Agency, Villanueva de la CaƱada (Madrid)

Written by C. Mignone/ESA