Several theories have attempted to explain why they don't show their age, but, until now, scientists have lacked the crucial observations with which to test each hypothesis.
Armed with such observational data, two astronomers from Northwestern University and the University of Wisconsin-Madison report that a mechanism known as mass transfer explains the origins of the blue stragglers.
Essentially, a blue straggler eats up the mass, or outer envelope, of its giant-star companion.
This extra fuel allows the straggler to continue to burn and live longer while the companion star is stripped bare, leaving only its white dwarf core.
The scientists report their evidence in a study to be published by the journal Nature.
The majority of blue stragglers in their study are in binaries: they have a companion star. "It's really the companion star that helped us determine where the blue straggler comes from," said Northwestern astronomer Aaron M. Geller, first author of the study.
"The companion stars orbit at periods of about 1,000 days, and we have evidence that the companions are white dwarfs. Both point directly to an origin from mass transfer."
Geller is the Lindheimer Postdoctoral Fellow in the Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and the department of physics and astronomy in Northwestern's Weinberg College of Arts and Sciences. Robert Mathieu, professor of astronomy and chair of the astronomy department at UW-Madison, is co-author of the study.
The astronomers studied the NGC 188 open cluster, which is in the constellation Cepheus, situated in the sky near Polaris, the North Star.
This cluster is one of the most ancient open star clusters, but it features these mysterious young blue stragglers.
The cluster has around 3,000 stars, all about the same age, and has 21 blue stragglers. Geller and Mathieu are the first to use detailed observational data from the WIYN Observatory in Tucson, Ariz., of the blue stragglers in NGC 188.
They used the information to analyze and compare the three main theories of blue straggler formation: collisions between stars, mergers of stars and mass transfer from one star to another. The only one left standing was the theory of mass transfer.
The light from the blue stragglers' companion stars is not actually visible in Geller and Mathieu's observations.
While the companions haven't been seen directly, their effect on the blue stragglers is evident: each companion pulls gravitationally on its blue straggler and creates a "wobble" as it orbits, and this allows astronomers to measure the mass of the companion stars.
The WIYN data show that each companion star is about half the mass of the sun, which is consistent with a white dwarf.
The other two origin theories, collisions and mergers, require the companion stars to be more massive than what is observed.
In fact, in both scenarios, some of the companion stars could be bright enough to be visible in the WIYN data, which is not the case.
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