Image Details

Choose export citation format:

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 7.

Comparison of αCO values estimated via different prescriptions (B13, SL24, and T24*, which represent Equations (8)–(10)). The dashed lines indicate a one-to-one relation, and the thick dotted lines label the Galactic αCO value of 4.35 ﹩{M}_{\odot }\,{({\rm{K}}\,\mathrm{km}\,{{\rm{s}}}^{-1}\,{\mathrm{pc}}^{2})}^{-1}﹩. While the predicted αCO values do not agree well and show no systematic trend among different populations, the overall αCO variations are limited to a factor of 2 within and among prescriptions. The fractional αCO uncertainty in these prescriptions is within ±0.2 dex for T24* and ±0.3 dex for B13 and SL24.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse