Figure 1 from Stellar and Molecular Gas Rotation in a Recently Quenched Massive Galaxy at z ∼ 0.7

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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 1.

(a) Median flux map of SDSS J0912+1523 from the Gemini spectra, with contours overlaid onto the Voronoi bins. (b) Full spectrum of the central Voronoi bin and the Hδ_A central bandpass, surrounded by blue and red “continuum” bandpasses, as defined by Worthey & Ottaviani (1997). The wavelengths of the [O II]λ3727, [O III]λ4959, and [O III]λ5007 lines are labeled.

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