The long-standing mystery of the origin of blue stragglers in globular clusters has been solved. Researchers have found that these overweight stars do not result primarily from collisions between stars but from stellar "cannibalism" in binary star systems where plasma is gradually pulled from one star to the other to form a more massive, bluer star.
A globular cluster is a spherical body composed of about 100,000 stars tightly bound by mutual gravity (CERN Courier July/August 2006 p10). Several tens of these clusters orbit our galaxy. They are usually composed of old stars all born at the same time in a giant star-formation region (CERN Courier June 2006 p14). In an old cluster, the most massive stars should have exhausted their hydrogen fuel a long time ago and should have died in supernova explosions. Only low-mass stars, shining redder light, should remain. However, globular clusters do contain several stars that are much too blue and too massive to have survived until now.
The origin of these "blue stragglers" that still fight for life has been a puzzle of stellar evolution for 55 years. As normal stellar formation cannot continue in globular clusters, owing to the quasi-absence of gas, there must be a different mechanism in their dense central cores that can continuously form massive stars. Two main theories emerged over time: that blue stragglers were created through collisions of two stars; or that one star in a binary system was "reborn" by pulling matter off its companion.
The new research by Christian Knigge from the University of Southampton, in the UK, and colleagues from McMaster University, in Canada, allows them to favour one of these scenarios. They compared the observed number of blue stragglers in 56 globular clusters with the predicted single–single stellar-collision rate based on the inner density of the clusters. They found no clear correlation, dispelling the theory that blue stragglers are created through collisions with other stars. On the other hand, they did find a strong relationship between the total mass contained in the core of the globular cluster and the number of blue stragglers observed within it. Because more massive cores also contain more binary stars, they inferred a connection between blue stragglers and binaries in globular clusters (Knigge et al. 2009).
This research provides strong evidence that the primary mechanism for the formation of blue stragglers is "stellar cannibalism" by the most massive star in a binary system as it pulls material from its lighter companion. What remains to be investigated is whether the binary parents of blue stragglers evolve mostly in isolation, or whether close encounters – failed collisions – with other stars in the cluster are required to form these binaries.