Figure 6 from The Kinematics of Ionized Gas in Lyman-break Analogs at z ∼ 0.2

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The Kinematics of Ionized Gas in Lyman-break Analogs at z ∼ 0.2

Authors: Thiago S. Gonçalves, Antara Basu-Zych, Roderik Overzier, D. Christopher Martin, David R. Law, David Schiminovich, Ted K. Wyder, Ryan Mallery, R. Michael Rich, and Timothy H. Heckman

GONÇALVES et al. 2010 The Astrophysical Journal 724 1373.

Provider: AAS Journals

Caption: Figure 6.

Ratio between dynamical and stellar masses as a function of stellar mass. Black filled circles indicate the LBAs in this paper, while the hollow red squares are the high- z LBGs from Law et al. (2009). The dashed line indicates M _dyn = M _*. More massive galaxies, both at low and high redshifts, present lower ratios, with M _dyn ~ 1/10 M _* for galaxies with log M _* ~ 10 ¹¹ M _☉.

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