Reconstructing the star formation history of the Milky Way disc(s) from chemical abundances

Owain Snaith(Centre National de la Recherche Scientifique), A. Gómez(Centre National de la Recherche Scientifique), D. Katz(Centre National de la Recherche Scientifique), F. Combes(Centre National de la Recherche Scientifique), P. Di Matteo(Observatoire de Paris), M. D. Lehnert(Centre National de la Recherche Scientifique), M. Haywood(Centre National de la Recherche Scientifique)
Astronomy and Astrophysics
March 20, 2015
10.1051/0004-6361/201424281
Cited by 187

Related Papers

The<i>Gaia</i>mission
|Astronomy and Astrophysics|2016|7k
<i>Gaia</i>Data Release 1
|Astronomy and Astrophysics|2016|2.1k
High molecular gas fractions in normal massive star-forming galaxies in the young Universe
|Nature|2010|991
A study of the gas-star formation relation over cosmic time★
|Monthly Notices of the Royal Astronomical Society|2010|952
PHIBSS: MOLECULAR GAS CONTENT AND SCALING RELATIONS IN<i>z</i>∼ 1-3 MASSIVE, MAIN-SEQUENCE STAR-FORMING GALAXIES
|The Astrophysical Journal|2013|941