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The EDGE-CALIFA Survey: Molecular Gas and Star Formation Activity across the Green Valley

  • Authors: Vicente Villanueva, Alberto D. Bolatto, Stuart N. Vogel, Tony Wong, Adam K. Leroy, Sebastian F. Sánchez, Rebecca C. Levy, Erik Rosolowsky, Dario Colombo, Veselina Kalinova, Serena Cronin, Peter Teuben, Mónica Rubio, Zein Bazzi

Vicente Villanueva et al 2024 The Astrophysical Journal 962 .

  • Provider: AAS Journals

Caption: Figure 3.

ACA EDGE data products for each galaxy. Panels cover an area of 1.′25 × 1.′25. The first column shows the SDSS riz multicolor image with contours from our integrated intensity masked map overlaid. Contours correspond to 2σ and 5σ CO(2−1) emission line levels. From left to right, the following columns show the CO(2−1) emission line intensity (moment 0, in units of Jy beam−1 km s−1), velocity (moment 1, in units of km s−1), and S/N peak maps, respectively. The red plus signs are the optical centers (columns (2) and (3) of Table 1). The black ellipses in the bottom left corner are the beam size of the CO(2−1) data. Panels for the remainder of the survey can be found in the Appendix.

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