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Stellar cannibalism is key to formation of overweight stars
Researchers have discovered that the mysterious overweight stars known as
blue stragglers are the result of 'stellar cannibalism' where plasma is
gradually pulled from one star to another to form a massive, unusually hot star
that appears younger than it is. The process takes place in binary stars - star
systems consisting of two stars orbiting around their common centre of mass.
This helps to resolve a long standing mystery in stellar evolution.

blue stragglers in globular cluster
Credit:NASA Goddard Space Flight Center
The research, which is part funded by the UK's Science and Technology
Facilities Council (STFC) and carried out by scientists at Southampton
University and the McMaster University in Canada, is published in the journal
Nature on Thursday 15 January.
Blue stragglers are found throughout the Universe in globular clusters -
collections of about 100, 000 stars, tightly bound by gravity. According to
conventional theories, the massive blue stragglers found in these clusters
should have died long ago because all stars in a cluster are born at the same
time and should therefore be at a similar phase. These massive rogue stars,
however, appear to be much younger than the other stars and are found in
virtually every observed cluster.
Dr Christian Knigge from Southampton University, who led the study,
comments: "The origin of blue stragglers has been a long-standing mystery. The
only thing that was clear is that at least two stars must be involved in the
creation of every single blue straggler, because isolated stars this massive
simply should not exist in these clusters.
Professor Alison Sills from the McMaster University explains further: "We've
known of these stellar anomalies for 55 years now. Over time two main theories
have emerged: that blue stragglers were created through collisions with other
stars; or that one star in a binary system was 'reborn' by pulling matter off
its companion.
The researchers looked at blue stragglers in 56 globular clusters. They
found that the total number of blue stragglers in a given cluster did not
correlate with predicted collision rate - dispelling the theory that blue
stragglers are created through collisions with other stars.
They did, however, discover a connection between the total mass contained in
the core of the globular cluster and the number of blue stragglers observed
within in. Since more massive cores also contain more binary stars, they were
able to infer a relationship between blue stragglers and binaries in globular
clusters. They also showed that this conclusion is supported by preliminary
observations that directly measured the abundance of binary stars in cluster
cores. All of this points to "stellar cannibalism" as the primary mechanism for
blue straggler formation.
Dr Knigge says: "This is the strongest and most direct evidence to date that
most blue stragglers, even those found in the cluster cores, are the offspring
of two binary stars. In our future work we will want to determine whether the
binary parents of blue stragglers evolve mostly in isolation, or whether
dynamical encounters with other stars in the clusters are required somewhere
along the line in order to explain our results."
This discovery comes as the world celebrates the International Year of
Astronomy in 2009.
Notes for editors
The research uses data taken with the Hubble Space Telescope
'A binary origin for 'blue stragglers' in globular clusters' is scheduled
for publication in Nature on 15 January.
Images
Contacts
- Julia
Short
STFC Press Officer
Tel: +44 (0) 1793 442012
- Glenn
Harris
Public Relations and Media Officer
University of Southampton
Tel: +44 (0)23 8059 3212
- Christian
Knigge
School of Physics & Astronomy
University of Southampton
Tel: +44-(0)23-8059-3955
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Page last updated: 16 January 2009
by Julia Short