Gas-phase metallicity gradients of TNG50 star-forming galaxies. Hemler, Z. S., Torrey, P., Qi, J., Hernquist, L., Vogelsberger, M., Ma, X., Kewley, L. J., Nelson, D., Pillepich, A., Pakmor, R., & Marinacci, F. arXiv e-prints, 2007:arXiv:2007.10993, July, 2020. ![Gas-phase metallicity gradients of TNG50 star-forming galaxies [link]](https://bibbase.org/img/filetypes/link.svg "link")
Paper abstract bibtex We present the radial gas-phase, mass-weighted metallicity profiles and gradients of the TNG50 star-forming galaxy population measured at redshifts \$z=\$ 0–3. We investigate the redshift evolution of gradients and examine relations between gradient steepness and galaxy properties. We find that TNG50 gradients are predominantly negative at all redshifts, although we observe significant diversity among these negative gradients. We determine that the gradient steepness of all galaxies increases approximately monotonically with redshift at a roughly constant rate. This rate does not vary significantly with galaxy mass. We observe a weak negative correlation between gradient steepness and galaxy stellar mass at redshifts \$z{\textbackslash}leq2\$. However, when we normalize gradients by a characteristic radius defined by the galactic star formation distribution, we find that these normalized gradients remain invariant with both stellar mass and redshift. We place our results in the context of previous simulations and show that TNG50 high-redshift gradients are steeper than those of models featuring burstier feedback, which may further highlight high-redshift gradients as important discriminators of galaxy formation models. We also find that redshift \$z=0\$ and \$z=0.5\$ TNG50 gradients are consistent with the gradients observed in galaxies at these redshifts, although the preference for flat gradients observed in redshift \$z{\textbackslash}gtrsim1\$ galaxies is not present in TNG50. If future JWST and ELT observations validate these flat gradients, it may indicate a need for simulation models to implement more powerful radial gas mixing within the ISM, possibly via turbulence and/or stronger winds
@article{hemler_gas-phase_2020,
title = {Gas-phase metallicity gradients of {TNG50} star-forming galaxies},
volume = {2007},
url = {http://adsabs.harvard.edu/abs/2020arXiv200710993H},
abstract = {We present the radial gas-phase, mass-weighted metallicity profiles and gradients of the TNG50 star-forming galaxy population measured at redshifts \$z=\$ 0--3. We investigate the redshift evolution of gradients and examine relations between gradient steepness and galaxy properties. We find that TNG50 gradients are predominantly negative at all
redshifts, although we observe significant diversity among these negative gradients. We determine that the gradient steepness of all galaxies increases approximately monotonically with redshift at a roughly constant rate. This rate does not vary significantly with galaxy mass. We observe a weak negative correlation between gradient steepness and galaxy stellar mass at redshifts \$z{\textbackslash}leq2\$. However, when we
normalize gradients by a characteristic radius defined by the galactic star formation distribution, we find that these normalized gradients remain invariant with both stellar mass and redshift. We place our results in the context of previous simulations and show that TNG50 high-redshift gradients are steeper than those of models featuring burstier feedback, which may further highlight high-redshift gradients as important discriminators of galaxy formation models. We also find that redshift \$z=0\$ and \$z=0.5\$ TNG50 gradients are consistent with the gradients observed in galaxies at these redshifts, although the
preference for flat gradients observed in redshift \$z{\textbackslash}gtrsim1\$ galaxies is not present in TNG50. If future JWST and ELT observations validate these flat gradients, it may indicate a need for simulation models to implement more powerful radial gas mixing within the ISM, possibly via turbulence and/or stronger winds},
urldate = {2020-07-24},
journal = {arXiv e-prints},
author = {Hemler, Z. S. and Torrey, Paul and Qi, Jia and Hernquist, Lars and Vogelsberger, Mark and Ma, Xiangcheng and Kewley, Lisa J. and Nelson, Dylan and Pillepich, Annalisa and Pakmor, Rüdiger and Marinacci, Federico},
month = jul,
year = {2020},
keywords = {Astrophysics - Astrophysics of Galaxies},
pages = {arXiv:2007.10993},
}
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We determine that the gradient steepness of all galaxies increases approximately monotonically with redshift at a roughly constant rate. This rate does not vary significantly with galaxy mass. We observe a weak negative correlation between gradient steepness and galaxy stellar mass at redshifts \\$z{\\textbackslash}leq2\\$. However, when we normalize gradients by a characteristic radius defined by the galactic star formation distribution, we find that these normalized gradients remain invariant with both stellar mass and redshift. We place our results in the context of previous simulations and show that TNG50 high-redshift gradients are steeper than those of models featuring burstier feedback, which may further highlight high-redshift gradients as important discriminators of galaxy formation models. We also find that redshift \\$z=0\\$ and \\$z=0.5\\$ TNG50 gradients are consistent with the gradients observed in galaxies at these redshifts, although the preference for flat gradients observed in redshift \\$z{\\textbackslash}gtrsim1\\$ galaxies is not present in TNG50. 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We investigate the redshift evolution of gradients and examine relations between gradient steepness and galaxy properties. We find that TNG50 gradients are predominantly negative at all\nredshifts, although we observe significant diversity among these negative gradients. We determine that the gradient steepness of all galaxies increases approximately monotonically with redshift at a roughly constant rate. This rate does not vary significantly with galaxy mass. We observe a weak negative correlation between gradient steepness and galaxy stellar mass at redshifts \\$z{\\textbackslash}leq2\\$. However, when we\nnormalize gradients by a characteristic radius defined by the galactic star formation distribution, we find that these normalized gradients remain invariant with both stellar mass and redshift. We place our results in the context of previous simulations and show that TNG50 high-redshift gradients are steeper than those of models featuring burstier feedback, which may further highlight high-redshift gradients as important discriminators of galaxy formation models. We also find that redshift \\$z=0\\$ and \\$z=0.5\\$ TNG50 gradients are consistent with the gradients observed in galaxies at these redshifts, although the\npreference for flat gradients observed in redshift \\$z{\\textbackslash}gtrsim1\\$ galaxies is not present in TNG50. If future JWST and ELT observations validate these flat gradients, it may indicate a need for simulation models to implement more powerful radial gas mixing within the ISM, possibly via turbulence and/or stronger winds},\n\turldate = {2020-07-24},\n\tjournal = {arXiv e-prints},\n\tauthor = {Hemler, Z. 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