International audienceWe report the first robust measurement of the Milky Way star formation history using the imprint left on chemical abundances of long-lived stars. The formation of the Galactic thick disk occurs during an intense star formation phase between 9.0 (z ~ 1.5) and 12.5 Gyr (z ~ 4.5) ago and is followed by a dip (at z ~ 1.1) lasting about 1 Gyr. Our results imply that the thick disk is as massive as the Milky Way's thin disk, suggesting a fundamental role of this component in the genesis of our Galaxy, something that had been largely unrecognized. This new picture implies that huge quantities of gas necessary to feed the building of the thick disk must have been present at these epochs, in contradiction with the long-term inf...
International audienceWe show that the bulge and the disk of the Milky Way (MW) at R ≲ 7 kpc are wel...
Many are the proposed scenarios for the formation of the thick disk of the Milky Way, goin...
Based on a physical treatment of the star formation law similar to that given by Efstathiou, we have...
International audienceWe report the first robust measurement of the Milky Way star formation history...
We report the first robust measurement of the Milky Way star formation history using the imprint lef...
International audienceWe analyze the chemical properties of a set of solar vicinity stars, and show ...
We develop a chemical evolution model to study the star formation history of the Milky Way. Our mode...
Detailed observations of the Milky Way can be used to test predictions from simulations of disk form...
We investigate thin and thick stellar disc formation in Milky Way-mass galaxies using 12 FIRE-2 cosm...
More than 30 years after its discovery, the thick disc of the Milky Way is not fully explored. We ex...
A chromospheric age distribution of 552 late-type dwarfs is transformed into a star formation histor...
The recently emerging conviction that thick disks are prevalent in disk galaxies, and their seemingl...
Aims. More than 30 years after its discovery, the thick disc of the Milky Way is not fully...
The disk galaxy simulated using our chemodynamic galaxy formation code, GCD+, is shown to have a thi...
The disk galaxy simulated using our chemodynamic galaxy formation code, GCD+, is shown to have a thi...
International audienceWe show that the bulge and the disk of the Milky Way (MW) at R ≲ 7 kpc are wel...
Many are the proposed scenarios for the formation of the thick disk of the Milky Way, goin...
Based on a physical treatment of the star formation law similar to that given by Efstathiou, we have...
International audienceWe report the first robust measurement of the Milky Way star formation history...
We report the first robust measurement of the Milky Way star formation history using the imprint lef...
International audienceWe analyze the chemical properties of a set of solar vicinity stars, and show ...
We develop a chemical evolution model to study the star formation history of the Milky Way. Our mode...
Detailed observations of the Milky Way can be used to test predictions from simulations of disk form...
We investigate thin and thick stellar disc formation in Milky Way-mass galaxies using 12 FIRE-2 cosm...
More than 30 years after its discovery, the thick disc of the Milky Way is not fully explored. We ex...
A chromospheric age distribution of 552 late-type dwarfs is transformed into a star formation histor...
The recently emerging conviction that thick disks are prevalent in disk galaxies, and their seemingl...
Aims. More than 30 years after its discovery, the thick disc of the Milky Way is not fully...
The disk galaxy simulated using our chemodynamic galaxy formation code, GCD+, is shown to have a thi...
The disk galaxy simulated using our chemodynamic galaxy formation code, GCD+, is shown to have a thi...
International audienceWe show that the bulge and the disk of the Milky Way (MW) at R ≲ 7 kpc are wel...
Many are the proposed scenarios for the formation of the thick disk of the Milky Way, goin...
Based on a physical treatment of the star formation law similar to that given by Efstathiou, we have...