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.

G. Germano Sacco, Rob Jeffries, Alex Binks, Laura Magrini, Francesco Damiani, Nicholas Wright, et al. (2023). The 4MOST Survey of Young Stars (4SYS). THE MESSENGER, 190, 7-9 [10.18727/0722-6691/5300].

The 4MOST Survey of Young Stars (4SYS)

Veronica Roccatagliata;
2023

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.
2023
G. Germano Sacco, Rob Jeffries, Alex Binks, Laura Magrini, Francesco Damiani, Nicholas Wright, et al. (2023). The 4MOST Survey of Young Stars (4SYS). THE MESSENGER, 190, 7-9 [10.18727/0722-6691/5300].
G. Germano Sacco; Rob Jeffries; Alex Binks; Laura Magrini; Francesco Damiani; Nicholas Wright; Loredana Prisinzano; Eleonora Zari; Christian Schneider...espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/977362
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