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Stars, Gas, and Star Formation of Distant Post-starburst Galaxies

  • Authors: Po-Feng Wu, 柏鋒 吳, Rachel Bezanson, Francesco D'Eugenio, Anna R. Gallazzi, Jenny E. Greene, Michael V. Maseda, Katherine A. Suess, Arjen van der Wel

Po-Feng Wu et al 2023 The Astrophysical Journal 955 .

  • Provider: AAS Journals

Caption: Figure 3.

The correlations between spectral indices and SFH parameters. The spectrum of LEGA-C 144377 does not cover the D n 4000 region. D n 4000 serves as a good qualitative proxy to the lookback time of the burst and the time that a galaxy became quiescent. On the other hand, there is no clear correlation between the burst strength and either D n 4000 or EW(Hδ). LEGA-C 144377 has not become quiescent (see the main text), we manually put it at t q = − 0.1.

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