Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift $\approx 3

Recent works identified a way to recover the time evolution of a galaxy's disk metallicity gradient from the shape of its age--metallicity relation. However, the success of the method is dependent on how the width of the star-forming region evolves over time, which in turn is dependent on a gal...

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Hauptverfasser: Ratcliffe, Bridget, Khoperskov, Sergey, Minchev, Ivan, Lee, Nathan D, Buck, Tobias, Marques, Léa, Lu, Lucy, Steinmetz, Matthias
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Sprache:eng
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