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Stellar and Molecular Gas Rotation in a Recently Quenched Massive Galaxy at z ∼ 0.7

  • Authors: Qiana Hunt, Rachel Bezanson, Jenny E. Greene, Justin S. Spilker, Katherine A. Suess, Mariska Kriek, Desika Narayanan, Robert Feldmann, Arjen van der Wel, and Petchara Pattarakijwanich

2018 The Astrophysical Journal Letters 860 L18.

  • Provider: AAS Journals

Caption: Figure 2.

Stellar kinematic and spectral index maps. The two flux peaks are marked with black + symbols. The seeing is indicated with gray bars. The left column shows the measured values of the (a) equivalent width of HδA, (b) velocity, and (c) velocity dispersion σ for each Voronoi bin. The middle column represents the estimated errors for each measurement. Velocity (row b) is measured with respect to the central bin, and its errors are presented as absolute values. The right column illustrates the relationship between the measured values and radial distance from the center of the galaxy. We omit outer bins below the target S/N = 6 in rows (a) and (c). These bins are blocked out in gray in the left column and by gray hashed boxes in the right column.

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