The Gaia-ESO Survey: A new approach to chemically characterising young open clusters

Baratella, M.; D'Orazi, V.; Sheminova, V.; Spina, L.; Carraro, G.; Gratton, R.; Magrini, L.; Randich, S.; Lugaro, M.; Pignatari, M.; Romano, D.; Biazzo, K.; Bragaglia, A.; Casali, G.; Desidera, S.; Frasca, A.; De Silva, G.; Melo, C.; Van Der Swaelmen, M.; Tautvaišienė, G.; Jiménez-Esteban, F. M.; Gilmore, G.; Bensby, T.; Smiljanic, R.; Bayo, A.; Franciosini, E.; Gonneau, A.; Hourihane, A.; Jofré, P.; Monaco, L.; Morbidelli, L.; Sacco, G.; Sbordone, L.; Worley, C.; Zaggia, S.

doi:10.1051/0004-6361/202141069

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The Gaia-ESO Survey: A new approach to chemically characterising young open clusters (2021)
Journal Article
Baratella, M., D'Orazi, V., Sheminova, V., Spina, L., Carraro, G., Gratton, R., …Zaggia, S. (2021). The Gaia-ESO Survey: A new approach to chemically characterising young open clusters. Astronomy and Astrophysics, 653, Article A67. https://doi.org/10.1051/0004-6361/202141069

Context. Young open clusters (ages of less than 200 Myr) have been observed to exhibit several peculiarities in their chemical compositions. These anomalies include a slightly sub-solar iron content, super-solar abundances of some atomic species (e.g... Read More about The Gaia-ESO Survey: A new approach to chemically characterising young open clusters.