Using ESO’s VLT Survey Telescope, a team of astronomers has found what looks like three different generations of baby stars within the Orion Nebula Cluster. This unexpected discovery adds very valuable new insights for the understanding of how such clusters form. It suggests that star formation might proceed in bursts, where each burst occurs on a much faster time-scale than previously thought.
OmegaCAM (the wide-field optical camera on ESO’s VLT Survey Telescope) has captured the spectacular Orion Nebula and its associated cluster of young stars in great detail, producing the beautiful new image shown at the top of the page. This object is one of the closest stellar nurseries for both low and high-mass stars, at a distance of about 1350 light-years.
But this is more than just a pretty picture. A team led by ESO astronomer Giacomo Beccari has used these data of unparalleled quality to precisely measure the brightness and colors of all the stars in the Orion Nebula Cluster. These measurements allowed the astronomers to determine the mass and ages of the stars. To their surprise, the data revealed three different sequences of potentially different ages.
“Looking at the data for the first time was one of those ‘Wow!’ moments that happen only once or twice in an astronomer’s lifetime,” says Beccari, lead author of the paper presenting the results. “The incredible quality of the OmegaCAM images revealed without any doubt that we were seeing three distinct populations of stars in the central parts of Orion.”
Monika Petr-Gotzens, co-author and also based at ESO Garching, continues, “This is an important result. What we are witnessing is that the stars of a cluster at the beginning of their lives didn’t form altogether simultaneously. This may mean that our understanding of how stars form in clusters needs to be modified.”
The astronomers looked carefully at the possibility that instead of indicating different ages, the different brightnesses and colors of some of the stars were due to hidden companion stars, which would make the stars appear brighter and redder than they really were. But this idea would imply quite unusual properties of the pairs, which have never before been observed. Other measurements of the stars, such as their rotation speeds and spectra, also indicated that they must have different ages.
This video sequence starts with a wide view of the Milky Way and slowly zooms in on the Orion Nebula, one of the brightest nearby regions of active star formation. The final view shows a very detailed new view of the stellar nursery from the VLT Survey Telescope.
“Although we cannot yet formally disprove the possibility that these stars are binaries, it seems much more natural to accept that what we see are three generations of stars that formed in succession, within less than three million years,” concludes Beccari.
The new results strongly suggest that star formation in the Orion Nebula Cluster is proceeding in bursts, and more quickly than had been previously thought.
Reference: “A Tale of Three Cities: OmegaCAM discovers multiple sequences in the color-magnitude diagram of the Orion Nebula Cluster” by G. Beccari, M. G. Petr-Gotzens, H. M. J. Boffin, M. Romaniello, D. Fedele, G. Carraro, G. De Marchi, W.-J. de Wit, J. E. Drew, V. M. Kalari, C. F. Manara, E. L. Martin, S. Mieske, N. Panagia, L. Testi, J. S. Vink, J. R. Walsh and N. J. Wright, 27 July 2017, Astronomy & Astrophysics.
DOI: 10.1051/0004-6361/201730432
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