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Close encounters of the stellar

IMAGE / NASA/CXC/MIT/D.Pooley et al. Globular cluster NGC 6266.


A team of scientists led by David Pooley of MIT took advantage of Chandra's unique ability to precisely locate and resolve individual sources to determine the number of X-ray sources in 12 globular clusters in our galaxy. Most of the sources are binary systems containing a collapsed star such as a neutronstar or a white dwarf star that is pulling matter off a normal, Sun-like companion star.


A similar study led by Craig Heinke of the Harvard-Smithsonian Center for Astrophysics confirmed this conclusion and showed that roughly 10 percent of these X-ray binary systems contain neutron stars. Most of these neutron stars are usually quiet, spending less than 10 percent of their time actively feeding from their companion.

A globular cluster is a spherical collection of hundreds of thousands or even millions of stars buzzing around each other in a gravitationally bound stellar beehive about a hundred light-years in diameter. The stars in a globular cluster are often only about a tenth of a light-year apart. For comparison, the nearest star to the Sun, Proxima Centauri, is 4.2 light-years away.


Observations by NASA's Uhuru X-ray satellite in the 1970s showed that globular clusters seemed to contain a disproportionately large number of X-ray binary sources compared to the galaxy as a whole. Normally only one in a billion stars is a member of an X-ray binary system containing a neutron star, whereas in globular clusters, the fraction is more like one in a million.

The present research confirms earlier suggestions that the chance of forming an X-ray binary system is dramatically increased by the congestion in a globular cluster. Under these conditions, two processes, known as three-star exchange collisions and tidal captures, can lead to a thousandfold increase in the number of X-ray sources in globular clusters.

In an exchange collision, a lone neutron star encounters a pair of ordinary stars. The intense gravity of the neutron star can induce the most massive ordinary star to "change partners" and pair up with the neutron star while ejecting the lighter star.

A neutron star could also have a grazing collision with a single normal star, and the intense gravity of the neutron star could distort the gravity of the normal star in the process. The energy lost in the distortion could prevent the normal star from escaping from the neutron star, leading to tidal capture.

In addition to solving a long-standing mystery, the Chandra data offer an opportunity for a deeper understanding of globular cluster evolution. "For example, the energy released in the formation of close binary systems could keep the central parts of the cluster from collapsing to form a massive black hole," Heinke said.

NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for NASA's Office of Space Science. The Smithsonian Astrophysical Observatory controls science and flight operations from the Chandra X-ray Center in Cambridge.

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