Full Screen Image
in the bulge of our galaxy
Massive stars live fast and furious, and hence the first generations of massive stars in the Universe are already dead. However, their chemical imprints, like fingerprints, can still be found today in the oldest stars in our Galaxy. These fossil records are thus the witnesses of the nature of the first stellar generations to pollute our Universe. “It is like if we tried to reveal the character of a cook from the taste of his dishes”, says Prof. Georges Meynet, from the Geneva University.
How were these first stars? Were they different from the stars we observe today?
Soon after the Big Bang, the composition of the Universe was much simpler than at present as it was made of essentially only hydrogen and helium. The chemical enrichment of the Universe with other elements had to wait around 300 million years until the fireworks started with the death of the first generations of massive stars, polluting the primordial gas with new chemical elements, which were later incorporated in the next generations of stars.
Using data from ESO’s Very Large Telescope (VLT), the astronomers reanalyzed spectra of a group of very old stars in the Galactic Bulge. These stars are so old that only very massive, short-living stars with masses larger than around ten times the mass of our Sun should have had time to die and to pollute the gas from which these fossil records then formed. As expected, the chemical composition of the observed stars showed elements typical for enrichment by massive stars. However, the new analysis unexpectedly also revealed elements usually thought to be produced only by stars of smaller masses. Fast-rotating massive stars on the other hand would succeed in manufacturing these elements themselves.
“Alternative scenarios cannot yet be discarded - but - we show that if the first generations of massive stars were spinstars, this would offer a very elegant explanation to this puzzle!”, says Cristina Chiappini. Team member Urs Frischknecht, a PhD student at the Basel University, is already working on extending the stellar simulations in order to further test the proposed scenario.
The impact of having had an early generation of spinstars in the Universe is manifold. Fast rotation also affects other properties of a star, such as its colour, its lifetime and its luminosity. Spinstars would therefore also have strongly influenced the properties and appearance of the first galaxies which were formed in the Universe. The existence of spinstars is now also supported by recent hydrodynamic simulations of the formation of the first stars of the universe by an independent research group.
Original publication: Chiappini et al., Imprints of fast-rotating massive stars in the Galactic Bulge, to be published in Nature, 2011. (DOI: 10.1038/nature10000, publication date: April 28, 2011)
Leibniz-Institut für Astrophysik Potsdam (AIP) - www.aip.de
Simulation of the formation of the first stars showing fast rotation (Credits: A. Stacy, University of Texas).
Dr. Cristina Chiappini, Leibniz-Institut für Astrophysik Potsdam (AIP), Email: email@example.com, Tel.: +49 331 7499 454
Dr. Gabriele Schönherr, Leibniz-Institut für Astrophysik Potsdam (AIP), Email: firstname.lastname@example.org, Tel.: +49 331 7499 383
Madleen Köppen, AIP, Email: email@example.com, Tel.: +49 331 7499 469
The key topics of the Leibniz Institute for Astrophysics (AIP) are cosmic magnetic fields and extragalactic astrophysics. A considerable part of the institute's efforts aim at the development of research technology in the fields of spectroscopy, robotic telescopes, and e-science. The AIP is the successor of the Berlin Observatory founded in 1700 and of the Astrophysical Observatory of Potsdam founded in 1874. The latter was the world's first observatory to emphasize explicitly the research area of astrophysics. The AIP is a foundation according to civil law and is a member of the Leibniz Association. The Leibniz Association is a network of 87 independent research institutes and scientific service facilities, which strive for scientific solutions for major social challenges.