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Star cluster discovery could upset the astronomical applecart

Last Updated on Tuesday, 07 March 2017 10:08
Published on Monday, 06 March 2017 16:30

The discovery of young stars in old star clusters could send scientists back to the drawing board for one of the Universe's most common objects. The new result appears in a paper in the journal Monthly Notices of the Royal Astronomical Society.

Dr Bi-Qing For, from the International Centre for Radio Astronomy Research (ICRAR) in Perth, Australia, said our understanding of how stars evolve is a cornerstone of astronomical science.

LMC Spitzer smallThis vibrant image from NASA’s Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. Credit: NASA/JPL-Caltech/M. Meixner (STScI) & the SAGE Legacy Team. Click for a full size image"There are a billion trillion stars in the Universe and we've been observing and classifying those we can see for more than a century," she said.

"Our models of stellar evolution are based on the assumption that stars within star clusters formed from the same material at roughly the same time."

A star cluster is a group of stars that share a common origin and are held together by gravity for some length of time. Because star clusters are assumed to contain stars of similar age and composition, researchers have used them as an "astronomical laboratory" to understand how mass affects the evolution of stars.

"If this assumption turns out to be incorrect, as our findings suggest, then these important models will need to be revisited and revised," said Dr For.

The discovery involves a study of star clusters located in the Large Magellanic Cloud, a neighbouring galaxy to the Milky Way.

By cross matching the locations of several thousand young stars with the locations of stellar clusters, the researchers found 15 stellar candidates that were much younger than other stars within the same cluster.

"The formation of these younger stars could have been fuelled by gas entering the clusters from interstellar space," said co-author Dr Kenji Bekki, also from ICRAR.

"But we eliminated this possibility using observations made by radio telescopes to show that there was no correlation between interstellar hydrogen gas and the location of the clusters we were studying.

"We believe the younger stars have actually been created out of the matter ejected from older stars as they die, which would mean we have discovered multiple generations of stars belonging to the same cluster."

LMC-Composite-smallThis image from NASA’s Spitzer Space Telescope features the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. Overlaying the image are circles showing the locations of 15 star clusters where multiple generations of stars have been discovered. Credit: Karl Gordon and Margaret Meixner – Space Telescope Science Institute/AURA/NASA. Compilation by Bi-Qing For and Kenji Bekki (ICRAR/UWA). Click for a full size imageDr Bekki said the stars were currently too faint to see using optical telescopes because of the dust that surrounds them.

"They have been observed using infrared wavelengths by orbiting space telescopes Spitzer and Herschel, operated by NASA and the European Space Agency," he said.

"An envelope of gas and dust surrounds these young stars but as they become more massive and this shroud blows away, they will become visible at optical wavelengths for powerful instruments like the Hubble Space Telescope."

"If we point Hubble at the clusters we've been studying, we should be able to see both young and old stars and confirm once and for all that star clusters can contain several generations of stars."

 

 

 

 

 

 

 

LMC-Composite-plus-Clusters-Pullout-smallLeft: This image from NASA’s Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. Overlaying the image are the locations of 15 star clusters where multiple generations of stars have been discovered. Right: A closer view of four of the star clusters where young stellar objects have been detected. The crosses mark the locations of young stars and the squares in the main image show the locations of these four clusters. Credit: Karl Gordon and Margaret Meixner – Space Telescope Science Institute/AURA/NASA. Compilation by Bi-Qing For and Kenji Bekki (ICRAR/UWA). Click for a full size image

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 


Media contacts

Pete Wheeler
ICRAR, Australia
Tel: +61 423 982 018
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Science contacts

Dr Bi-Qing For
ICRAR-UWA, Australia
Tel: +61 08 6488 7729
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Dr Kenji Bekki
ICRAR-UWA, Australia
Tel: +61 08 6488 7730
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Further information

The work appears in 'A discovery of young stellar objects in older clusters of the Large Magellanic Cloud', Bi-Qing For and Kenji Bekki, Monthly Notices of the Royal Astronomical Society, Oxford University Press.

 


Notes for editors

The International Centre for Radio Astronomy Research (ICRAR) is a joint venture between Curtin University and The University of Western Australia with support and funding from the State Government of Western Australia.

The Royal Astronomical Society, founded in 1820, encourages and promotes the study of astronomy, solar-system science, geophysics and closely related branches of science. The RAS organizes scientific meetings, publishes international research and review journals, recognizes outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 4,000 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.

The RAS accepts papers for its journals based on the principle of peer review, in which fellow experts on the editorial boards accept the paper as worth considering. The Society issues press releases based on a similar principle, but the organisations and scientists concerned have overall responsibility for their content.

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