1. Gas outflows in two recently quenched galaxies at z = 4 and 7
- Author
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Valentino, F., Heintz, K. E., Brammer, G., Ito, K., Kokorev, V., Whitaker, K. E., Gallazzi, A., de Graaff, A., Weibel, A., Frye, B. L., Kamieneski, P. S., Jin, S., Ceverino, D., Faisst, A., Farcy, M., Fujimoto, S., Gillman, S., Gottumukkala, R., Hamadouche, M., Harrington, K. C., Hirschmann, M., Jespersen, C. K., Kakimoto, T., Kubo, M., Lagos, C. d. P., Lee, M., Magdis, G. E., Man, A. W. S., Onodera, M., Rizzo, F., Shimakawa, R., Setton, D. J., Tanaka, M., Toft, S., Wu, P. -F., and Zhu, P.
- Subjects
Astrophysics - Astrophysics of Galaxies ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
Outflows are a key element in the baryon cycle of galaxies, and their properties provide a fundamental test for our models of how star formation quenches in galaxies. Here we report the detection of outflowing gas in two recently quenched, massive ($M_\star\sim10^{10.2}M_\odot$) galaxies at z=4.106 (NS_274) and z=7.276 (RUBIES-UDS-QG-z7) observed with JWST/NIRSpec. The outflows are traced by blue-shifted MgII absorption lines, and in the case of the z=4.1 system, also by FeII and NaI features. The spectra of the two sources are similar to those of local post-starburst galaxies, showing deep Balmer features and minimal star formation on 10 Myr timescales as traced by the lack of bright emission lines, also suggesting the absence of a strong and radiatively efficient AGN. The galaxies' SFHs are consistent with an abrupt quenching of star formation, which continued at rates of $\sim15\,M_\odot$/yr averaged over 100 Myr timescales. Dedicated millimeter observations of NS_274 constrain its dust obscured SFR to $<12\,M_\odot$/yr. Under simple geometrical assumptions, we derive mass loading factors $\lesssim1$ and $\sim50$ for the z=4.1 and z=7.3 systems, respectively, and similarly different energies carried by the outflows. Supernovae feedback can account for the mass and energy of the outflow in NS_274. However, the low mass loading factor and average gas velocity suggest that the observed outflow is unlikely to be the reason behind its quenching. SF-related processes seem to be insufficient to explain the extreme mass outflow rate of RUBIES-UDS-QG-z7, which would require an additional ejective mechanism such as an undetected AGN. Finally, the average outflow velocities per unit $M_\star$, SFR, or its surface area are consistent with those of lower-redshift post-starburst galaxies, suggesting that outflows in rapidly quenched galaxies might occur similarly across cosmic time. [Abridged], Comment: 13 pages, 7 figures + Appendix. Submitted to A&A on Jan 27, 2025. See Ito et al. (2025) on arXiv today for another result from the JWST "DeepDive" program
- Published
- 2025