SMC in space and time: a project to study the evolution of the prototype interacting late-type dwarf galaxy
conference contribution
posted on 2023-05-23, 16:59authored byTosi, M, Gallagher, J, Sabbi, E, Glatt, K, Grebel, EK, Christian, C, Cignoni, M, Clementini, G, Andrew ColeAndrew Cole, Da Costa, G, Harbeck, D, Marconi, M, Meixner, M, Nota, A, Sirianni, M, Smecker-Hane, T
We introduce the SMC in space and time, a large coordinated space and ground-based program to study star formation processes and history, as well as variable stars, structure, kinematics and chemical evolution of the whole SMC. Here, we present the Colour-Magnitude Diagrams (CMDs) resulting from HST/ACS photometry, aimed at deriving the star formation history (SFH) in six fields of the SMC. The fields are located in the central regions, in the stellar halo, and in the wing toward the LMC. The CMDs are very deep, well beyond the oldest Main Sequence Turn-Off, and will allow us to derive the SFH over the entire Hubble time.
History
Publication title
Low-Metallicity Star Formation: From Stars to Dwarf Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 255
Volume
4
Editors
LK Hunt, S Madden and R Schneider
Pagination
381-386
ISBN
9780521889865
Department/School
School of Natural Sciences
Publisher
Cambridge University Press
Place of publication
London
Event title
Low-Metallicity Star Formation: From the First Stars to Dwarf Galaxies, IAU Symposium S255