The synchronized dance of the magellanic clouds' star formation history

We use the SMASH survey to obtain unprecedented deep photometry reaching down to the oldest main-sequence turn-offs in the colour-magnitude diagrams (CMDs) of the Small Magellanic Cloud (SMC) and quantitatively derive its star formation history (SFH) using CMD fitting techniques. We identify five di...

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Bibliographic Details
Main Authors: Bernard, E.J (Author), Besla, G. (Author), Cassisi, S. (Author), Choi, Y. (Author), Cioni, M.-R.L (Author), De Boer, T.J.L (Author), Dorta, A. (Author), Gallart, C. (Author), Massana, P. (Author), Monachesi, A. (Author), Monelli, M. (Author), Nidever, D.L (Author), Noël, N.E.D (Author), Olsen, K.A.G (Author), Ruiz-Lara, T. (Author), Sakowska, J.D (Author), Stringfellow, G.S (Author), Van Der Marel, R.P (Author), Walker, A.R (Author), Zaritsky, D. (Author)
Format: Article
Language:English
Published: Oxford University Press 2022
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