Figure 8 from The Molecular Gas Content and Fuel Efficiency of Starbursts at z ∼ 1.6 with ALMA

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The Molecular Gas Content and Fuel Efficiency of Starbursts at z ∼ 1.6 with ALMA

Authors: J. D. Silverman, W. Rujopakarn, E. Daddi, A. Renzini, G. Rodighiero, D. Liu, A. Puglisi, M. Sargent, C. Mancini, J. Kartaltepe, D. Kashino, A. Koekemoer, N. Arimoto, M. Béthermin, S. Jin, G. Magdis, T. Nagao, M. Onodera, D. Sanders, and F. Valentino

2018 The Astrophysical Journal 867 92.

Provider: AAS Journals

Caption: Figure 8.

(a) Gas depletion time (τ_depl = M_gas/SFR) of high-redshift starbursts as a function of their SFR. The slanted black line is the best-fit relation from Sargent et al. (2014). (b) Gas depletion time vs. sSFR with both normalized to average values for SF MS galaxies. An analytic form of this relation is provided by Tacconi et al. (2017) and shown here in green. Symbols in both panels are the same as in Figure 6.

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