C. R. Boxer, "The Dutch in Brazil, 1624-1654" (Book Review)

Lyman-α at Cosmic Noon II: The relationship between kinematics and Lyman-α in z ∼ 2–3 Lyman break galaxies

“…The synthesis of these results has produced a picture of the high-redshift SFG population in which the majority ( 75%) of massive ( ) SFGs appear to have assembled primitive discs with characteristically large ionised gas velocity dispersions and rotation-dominated kinematics (e.g., Wisnioski et al 2015, 2019; Simons et al 2016, 2017; Förster Schreiber et al 2018). Lensed and other deep surveys targeting lower mass ( ) SFGs report a significantly lower ( 50%) rotation-dominated fraction and a higher proportion of galaxies that are kinematically disordered (dispersion-dominated) or have kinematic structure and/or morphologies that identified them as mergers (e.g., Gnerucci et al 2011; Livermore et al 2015; Leethochawalit et al 2016; Mason et al 2017; Turner et al 2017; Girard et al 2018). Additionally, the nebular emission-line kinematics of SFGs in the redshift range , have been shown to correlate with a range of galactic physical properties including: stellar and dynamical mass; size and morphology; specific and total star formation rates; gas outflows and gas fraction; and nebular conditions including the degree and spatial distribution of metals (see for example Glazebrook 2013 and references therein, and more recently, Wisnioski et al 2015, 2018, 2019; Leethochawalit et al 2016; Simons et al 2016, 2017; Mason et al 2017; Molina et al 2017; Turner et al 2017; Girard et al 2018; Förster Schreiber et al 2018, 2019; and Förster Schreiber & Wuyts 2020).…”