DUVET: sub-kiloparsec resolved star formation driven outflows in a sample of local starbursting disk galaxies

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Hauptverfasser: Chu, Bronwyn Reichardt, Fisher, Deanne B., Chisholm, John, Berg, Danielle, Bolatto, Alberto, Cameron, Alex J., Fielding, Drummond B., Herrera-Camus, Rodrigo, Kacprzak, Glenn G., Li, Miao, McLeod, Anna F., McPherson, Daniel K., Nielsen, Nikole M., Vaught, Ryan Rickards, Ridolfo, Sophia G., Sandstrom, Karin
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Veröffentlicht: 2024
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author Chu, Bronwyn Reichardt
Fisher, Deanne B.
Chisholm, John
Berg, Danielle
Bolatto, Alberto
Cameron, Alex J.
Fielding, Drummond B.
Herrera-Camus, Rodrigo
Kacprzak, Glenn G.
Li, Miao
McLeod, Anna F.
McPherson, Daniel K.
Nielsen, Nikole M.
Vaught, Ryan Rickards
Ridolfo, Sophia G.
Sandstrom, Karin
author_facet Chu, Bronwyn Reichardt
Fisher, Deanne B.
Chisholm, John
Berg, Danielle
Bolatto, Alberto
Cameron, Alex J.
Fielding, Drummond B.
Herrera-Camus, Rodrigo
Kacprzak, Glenn G.
Li, Miao
McLeod, Anna F.
McPherson, Daniel K.
Nielsen, Nikole M.
Vaught, Ryan Rickards
Ridolfo, Sophia G.
Sandstrom, Karin
contents We measure resolved (kiloparsec-scale) outflow properties in a sample of 10 starburst galaxies from the DUVET (Deep near-UV observations of Entrained gas in Turbulent galaxies) sample, using Keck/KCWI observations of H$β$ and [OIII]~$λ$5007. We measure $\sim460$ lines-of-sight that contain outflows, and use these to study scaling relationships of outflow velocity ($v_{\rm out}$), mass-loading factor ($η$; mass outflow rate per SFR) and mass flux ($\dotΣ_{\rm out}$; mass outflow rate per area) with co-located SFR surface density ($Σ_{\rm SFR}$) and stellar mass surface density ($Σ_{\ast}$). We find strong, positive correlations of $\dotΣ_{\rm out} \propto Σ_{\rm SFR}^{1.2}$ and $\dotΣ_{\rm out} \propto Σ_{\ast}^{1.5}$. We also find shallow correlations between $v_{\rm out}$ and both $Σ_{\rm SFR}$ and $Σ_{\ast}$. Our resolved observations do not suggest a threshold in outflows with $Σ_{\rm SFR}$, but rather we find that the local specific SFR ($Σ_{\rm SFR}/Σ_\ast$) is a better predictor of where outflows are detected. We find that outflows are very common above $Σ_{\rm SFR}/Σ_\ast\gtrsim 0.1$~Gyr$^{-1}$ and rare below this value. We argue that our results are consistent with a picture in which outflows are driven by supernovae, and require more significant injected energy in higher mass surface density environments to overcome local gravity. The correlations we present here provide a statistically robust, direct comparison for simulations and higher redshift results from JWST.
format Preprint
id arxiv_https___arxiv_org_abs_2402_17830
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle DUVET: sub-kiloparsec resolved star formation driven outflows in a sample of local starbursting disk galaxies
Chu, Bronwyn Reichardt
Fisher, Deanne B.
Chisholm, John
Berg, Danielle
Bolatto, Alberto
Cameron, Alex J.
Fielding, Drummond B.
Herrera-Camus, Rodrigo
Kacprzak, Glenn G.
Li, Miao
McLeod, Anna F.
McPherson, Daniel K.
Nielsen, Nikole M.
Vaught, Ryan Rickards
Ridolfo, Sophia G.
Sandstrom, Karin
Astrophysics of Galaxies
We measure resolved (kiloparsec-scale) outflow properties in a sample of 10 starburst galaxies from the DUVET (Deep near-UV observations of Entrained gas in Turbulent galaxies) sample, using Keck/KCWI observations of H$β$ and [OIII]~$λ$5007. We measure $\sim460$ lines-of-sight that contain outflows, and use these to study scaling relationships of outflow velocity ($v_{\rm out}$), mass-loading factor ($η$; mass outflow rate per SFR) and mass flux ($\dotΣ_{\rm out}$; mass outflow rate per area) with co-located SFR surface density ($Σ_{\rm SFR}$) and stellar mass surface density ($Σ_{\ast}$). We find strong, positive correlations of $\dotΣ_{\rm out} \propto Σ_{\rm SFR}^{1.2}$ and $\dotΣ_{\rm out} \propto Σ_{\ast}^{1.5}$. We also find shallow correlations between $v_{\rm out}$ and both $Σ_{\rm SFR}$ and $Σ_{\ast}$. Our resolved observations do not suggest a threshold in outflows with $Σ_{\rm SFR}$, but rather we find that the local specific SFR ($Σ_{\rm SFR}/Σ_\ast$) is a better predictor of where outflows are detected. We find that outflows are very common above $Σ_{\rm SFR}/Σ_\ast\gtrsim 0.1$~Gyr$^{-1}$ and rare below this value. We argue that our results are consistent with a picture in which outflows are driven by supernovae, and require more significant injected energy in higher mass surface density environments to overcome local gravity. The correlations we present here provide a statistically robust, direct comparison for simulations and higher redshift results from JWST.
title DUVET: sub-kiloparsec resolved star formation driven outflows in a sample of local starbursting disk galaxies
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2402.17830