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The EDGE-CALIFA Survey: Star Formation Efficiency and Galaxy Quenching across 62 Main-sequence, Green Valley, and Red Galaxies

  • Authors: Yu-Hsuan Teng, Alberto D. Bolatto, Peter J. Teuben, Erik Rosolowsky, David T. Frayer, Amanda A. Kepley, Sebastian F. Sanchez, Tony Wong, Adam K. Leroy, Dario Colombo, Serena A. Cronin, K. Decker French, Veselina Kalinova, Rebecca C. Levy, Karin M. Sandstrom, Vicente Villanueva, Jorge K. Barrera-Ballesteros, Zein Bazzi, Yixian Cao, Alex Green, Rodrigo Herrera-Camus, Eduardo A. D. Lacerda, Jialu Li, Alejandra Z. Lugo-Aranda, Jocabed Martinez-Lopez, Elizabeth Tarantino, Akshat Tripathi, Carolyn G. Volpert, Di Wen

Yu-Hsuan Teng et al 2026 The Astrophysical Journal 1007 .

  • Provider: AAS Journals

Caption: Figure 12.

Same as Figure 8 but using Mmol and tdep derived via the B13 (left), SL24 (middle), and T24* (right) αCO prescriptions. The best-fit slopes for quenched galaxies (red dashed lines) are −0.49, −0.48, and −0.41 for B13, SL24, and T24*, respectively. The qualitative results remain the same as using a constant αCO, as the αCO variation within and among prescriptions is small compared to the orders-of-magnitude span in tdep, and there is no systematic αCO dependence on ΔSFMS.

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