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 Alves; Amelia 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

doi:10.18727/0722-6691/5300

Amelia 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

Department of Astrophysics

Publications: Contribution to journal › Article

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 language	English
Pages (from-to)	7-9
Number of pages	3
Journal	The Messenger
Volume	190
DOIs	https://doi.org/10.18727/0722-6691/5300
Publication status	Published - Mar 2023

Austrian Fields of Science 2012

103003 Astronomy
103004 Astrophysics

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Sacco, G. G., Jeffries, R. D., Binks, A. S., Magrini, L., Damiani, F., Wright, N. J., Prisinzano, L., Zari, E., Schneider, C., Beccari, G., Weaver, G., D’Orazi, V., Biazzo, K., Nisini, B., Antoniucci, S., Franciosini, E., Robrade, J., Stelzer, B., Alfaro, E. J., ... Spina, L. (2023). The 4MOST Survey of Young Stars (4SYS). The Messenger, 190, 7-9. https://doi.org/10.18727/0722-6691/5300

@article{5d34bba643e7402bae9cfbc9f944dca7,

title = "The 4MOST Survey of Young Stars (4SYS)",

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. ",

author = "Sacco, \{Giuseppe Germano\} and Jeffries, \{R. D.\} and Binks, \{A. S.\} and L. Magrini and Francesco Damiani and Wright, \{N. J.\} and L. Prisinzano and E. Zari and C. Schneider and G. Beccari and G. Weaver and V. D{\textquoteright}Orazi and Katia Biazzo and B. Nisini and S. Antoniucci and E. Franciosini and J. Robrade and B. Stelzer and Alfaro, \{E. J.\} and Joao Alves and Amelia Bayo and Boffin, \{H. M. J.\} and Rosaria Bonito and Herv{\'e} Bouy and Brown, \{Anthony G.A.\} and E. Corbelli and S. Degl'Innocenti and D. Fedele and Jonathan Gagne and P. Galli and Gro{\ss}schedl, \{Josefa Elisabeth\} and T. Jerabkova and Kastner, \{Joel H.\} and D. Kawata and Stefan Meingast and \{Miret Roig\}, N{\'u}ria and Estelle Moraux and Javier Olivares and Parker, \{Richard J.\} and P.G.P. Moroni and Timo Prusti and S. Randich and V. Roccatagliata and Lorenzo Spina",

year = "2023",

month = mar,

doi = "10.18727/0722-6691/5300",

language = "English",

volume = "190",

pages = "7--9",

journal = "The Messenger",

issn = "0722-6691",

publisher = "ESO",

}

Sacco, GG, Jeffries, RD, Binks, AS, Magrini, L, Damiani, F, Wright, NJ, Prisinzano, L, Zari, E, Schneider, C, Beccari, G, Weaver, G, D’Orazi, V, Biazzo, K, Nisini, B, Antoniucci, S, Franciosini, E, Robrade, J, Stelzer, B, Alfaro, EJ, Alves, J, Bayo, A, Boffin, HMJ, Bonito, R, Bouy, H, Brown, AGA, Corbelli, E, Degl'Innocenti, S, Fedele, D, Gagne, J, Galli, P, Großschedl, JE, Jerabkova, T, Kastner, JH, Kawata, D, Meingast, S, Miret Roig, N, Moraux, E, Olivares, J, Parker, RJ, Moroni, PGP, Prusti, T, Randich, S, Roccatagliata, V & Spina, L 2023, 'The 4MOST Survey of Young Stars (4SYS)', The Messenger, vol. 190, pp. 7-9. https://doi.org/10.18727/0722-6691/5300

TY - JOUR

T1 - The 4MOST Survey of Young Stars (4SYS)

AU - Sacco, Giuseppe Germano

AU - Jeffries, R. D.

AU - Binks, A. S.

AU - Magrini, L.

AU - Damiani, Francesco

AU - Wright, N. J.

AU - Prisinzano, L.

AU - Zari, E.

AU - Schneider, C.

AU - Beccari, G.

AU - Weaver, G.

AU - D’Orazi, V.

AU - Biazzo, Katia

AU - Nisini, B.

AU - Antoniucci, S.

AU - Franciosini, E.

AU - Robrade, J.

AU - Stelzer, B.

AU - Alfaro, E. J.

AU - Alves, Joao

AU - Bayo, Amelia

AU - Boffin, H. M. J.

AU - Bonito, Rosaria

AU - Bouy, Hervé

AU - Brown, Anthony G.A.

AU - Corbelli, E.

AU - Degl'Innocenti, S.

AU - Fedele, D.

AU - Gagne, Jonathan

AU - Galli, P.

AU - Großschedl, Josefa Elisabeth

AU - Jerabkova, T.

AU - Kastner, Joel H.

AU - Kawata, D.

AU - Meingast, Stefan

AU - Miret Roig, Núria

AU - Moraux, Estelle

AU - Olivares, Javier

AU - Parker, Richard J.

AU - Moroni, P.G.P.

AU - Prusti, Timo

AU - Randich, S.

AU - Roccatagliata, V.

AU - Spina, Lorenzo

PY - 2023/3

Y1 - 2023/3

N2 - 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.

AB - 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.

U2 - 10.18727/0722-6691/5300

DO - 10.18727/0722-6691/5300

M3 - Article

SN - 0722-6691

VL - 190

SP - 7

EP - 9

JO - The Messenger

JF - The Messenger

ER -

The 4MOST Survey of Young Stars (4SYS)

Abstract

Austrian Fields of Science 2012

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