The 4MOST Survey of Young Stars (4SYS)

Giuseppe Germano Sacco, R. D. Jeffries, A. S. Binks, L. Magrini, Francesco Damiani, N. J. Wright, L. Prisinzano, E. Zari, C. Schneider, G. Beccari, G. Weaver, V. D’Orazi, Katia Biazzo, B. Nisini, S. Antoniucci, E. Franciosini, J. Robrade, B. Stelzer, E. J. Alfaro, Joao AlvesAmelia Bayo, H. M. J. Boffin, Rosaria Bonito, Hervé Bouy, Anthony G.A. Brown, E. Corbelli, S. Degl'Innocenti, D. Fedele, Jonathan Gagne, P. Galli, Josefa Elisabeth Großschedl, T. Jerabkova, Joel H. Kastner, D. Kawata, Stefan Meingast, Núria Miret Roig, Estelle Moraux, Javier Olivares, Richard J. Parker, P.G.P. Moroni, Timo Prusti, S. Randich, V. Roccatagliata, Lorenzo Spina

Publications: Contribution to journalArticle

Abstract

Most nearby young stars (with ages < 100 Myr) in the Galactic disc no longer reside in their dense, clustered birthplaces; they are found all around us. The 4MOST Survey of Young Stars will identify a representative sample of about 105 young, low-mass stars within 500 pc of the Sun and will measure their chemistry, 3D kinematics and ages in order to: trace the spatial and dynamical evolution of star-forming structures; quantify the star formation rate and chemical inhomogeneity in the local disc; vastly expand the number of identified young stars for exoplanetary studies; and provide huge coeval samples to improve young stellar evolutionary models.
Original languageEnglish
Pages (from-to)7-9
Number of pages3
JournalThe Messenger
Volume190
DOIs
Publication statusPublished - Mar 2023

Austrian Fields of Science 2012

  • 103003 Astronomy
  • 103004 Astrophysics

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