Gas kinematics, morphology and angular momentum in the FIRE simulations
Abstract
We report on the z = 0 gas kinematics, morphology and angular momentum content of isolated galaxies in a suite of cosmological zoom-in simulations from the FIRE project spanning Mstar = 106–11 M⊙. Gas becomes increasingly rotationally supported with increasing galaxy mass. In the lowest mass galaxies (Mstar < 108M⊙), gas fails to form a morphological disc and is primarily dispersion and pressure supported. At intermediate masses (Mstar = 108–10 M⊙), galaxies display a wide range of gas kinematics and morphologies, from thin, rotating discs to irregular spheroids with negligible net rotation. All the high-mass (Mstar = 1010–11 M⊙) galaxies form rotationally supported gas discs. Many of the haloes whose galaxies fail to form discs harbour high angular momentum gas in their circumgalactic medium. The ratio of the specific angular momentum of gas in the central galaxy to that of the dark matter halo increases significantly with galaxy mass, from $$\langle$$jgas$$\rangle$$$$\langle$$jDM$$\rangle$$ ~ 0.1 at Mstar=106--7M⊙ to$$\langle$$gas$$\rangle$$/$$\langle$$jDM$$\rangle$$ ~ 2 at Mstar = 1010–11 M⊙. The reduced rotational support in the lowest mass galaxies owes to (a) stellar feedback and the UV background suppressing the accretion of high angular momentum gas at late times, and (b) stellar feedback driving large non-circular gas motions. We broadly repeat the observed scaling relations between galaxy mass, gas rotation velocity, size and angular momentum, but may somewhat underpredict the incidence of disky, high angular momentum galaxies at the lowest observed masses (Mstar = (106-2× 107) M⊙). Stars form preferentially from low angular momentum gas near the galactic centre and are less rotationally supported than gas. The common assumption that stars follow the same rotation curve as gas thus substantially overestimates the simulated galaxies’ stellar angular momentum, particularly at low masses.
- Authors:
-
[1];
[3];
[1];
[3]
- Univ. of California, Berkeley, CA (United States)
- California Inst. of Technology (CalTech), Pasadena, CA (United States); Observatories of the Carnegie Inst. for Science, Pasadena, CA (United States); Univ. of California, Davis, CA (United States)
- California Inst. of Technology (CalTech), Pasadena, CA (United States)
- Univ. of California, San Diego, CA (United States)
- Univ. of Texas, Austin, TX (United States)
- Northwestern Univ., Evanston, IL (United States)
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1523825
- Grant/Contract Number:
- AC02-05CH11231
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Monthly Notices of the Royal Astronomical Society
- Additional Journal Information:
- Journal Volume: 473; Journal Issue: 2; Journal ID: ISSN 0035-8711
- Publisher:
- Royal Astronomical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; galaxies: dwarf; galaxies: irregular; galaxies: kinematics and dynamics
Citation Formats
El-Badry, Kareem, Quataert, Eliot, Wetzel, Andrew, Hopkins, Philip F., Weisz, Daniel R., Chan, T. K., Fitts, Alex, Boylan-Kolchin, Michael, Kereš, Dušan, Faucher-Giguère, Claude-André, and Garrison-Kimmel, Shea. Gas kinematics, morphology and angular momentum in the FIRE simulations. United States: N. p., 2017.
Web. doi:10.1093/mnras/stx2482.
El-Badry, Kareem, Quataert, Eliot, Wetzel, Andrew, Hopkins, Philip F., Weisz, Daniel R., Chan, T. K., Fitts, Alex, Boylan-Kolchin, Michael, Kereš, Dušan, Faucher-Giguère, Claude-André, & Garrison-Kimmel, Shea. Gas kinematics, morphology and angular momentum in the FIRE simulations. United States. https://doi.org/10.1093/mnras/stx2482
El-Badry, Kareem, Quataert, Eliot, Wetzel, Andrew, Hopkins, Philip F., Weisz, Daniel R., Chan, T. K., Fitts, Alex, Boylan-Kolchin, Michael, Kereš, Dušan, Faucher-Giguère, Claude-André, and Garrison-Kimmel, Shea. Tue .
"Gas kinematics, morphology and angular momentum in the FIRE simulations". United States. https://doi.org/10.1093/mnras/stx2482. https://www.osti.gov/servlets/purl/1523825.
@article{osti_1523825,
title = {Gas kinematics, morphology and angular momentum in the FIRE simulations},
author = {El-Badry, Kareem and Quataert, Eliot and Wetzel, Andrew and Hopkins, Philip F. and Weisz, Daniel R. and Chan, T. K. and Fitts, Alex and Boylan-Kolchin, Michael and Kereš, Dušan and Faucher-Giguère, Claude-André and Garrison-Kimmel, Shea},
abstractNote = {We report on the z = 0 gas kinematics, morphology and angular momentum content of isolated galaxies in a suite of cosmological zoom-in simulations from the FIRE project spanning Mstar = 106–11 M⊙. Gas becomes increasingly rotationally supported with increasing galaxy mass. In the lowest mass galaxies (Mstar < 108M⊙), gas fails to form a morphological disc and is primarily dispersion and pressure supported. At intermediate masses (Mstar = 108–10 M⊙), galaxies display a wide range of gas kinematics and morphologies, from thin, rotating discs to irregular spheroids with negligible net rotation. All the high-mass (Mstar = 1010–11 M⊙) galaxies form rotationally supported gas discs. Many of the haloes whose galaxies fail to form discs harbour high angular momentum gas in their circumgalactic medium. The ratio of the specific angular momentum of gas in the central galaxy to that of the dark matter halo increases significantly with galaxy mass, from $\langle$jgas$\rangle$$\langle$jDM$\rangle$ ~ 0.1 at Mstar=106--7M⊙ to$\langle$gas$\rangle$/$\langle$jDM$\rangle$ ~ 2 at Mstar = 1010–11 M⊙. The reduced rotational support in the lowest mass galaxies owes to (a) stellar feedback and the UV background suppressing the accretion of high angular momentum gas at late times, and (b) stellar feedback driving large non-circular gas motions. We broadly repeat the observed scaling relations between galaxy mass, gas rotation velocity, size and angular momentum, but may somewhat underpredict the incidence of disky, high angular momentum galaxies at the lowest observed masses (Mstar = (106-2× 107) M⊙). Stars form preferentially from low angular momentum gas near the galactic centre and are less rotationally supported than gas. The common assumption that stars follow the same rotation curve as gas thus substantially overestimates the simulated galaxies’ stellar angular momentum, particularly at low masses.},
doi = {10.1093/mnras/stx2482},
journal = {Monthly Notices of the Royal Astronomical Society},
number = 2,
volume = 473,
place = {United States},
year = {Tue Sep 26 00:00:00 EDT 2017},
month = {Tue Sep 26 00:00:00 EDT 2017}
}
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Figures / Tables:
Table 1: Summary of the simulations at $z$ = 0.
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Evolution of the Three-dimensional Shape of Passively Evolving and Star-forming Galaxies at z < 1
journal, November 2019
- Satoh, Yuki K.; Kajisawa, Masaru; Himoto, Kazuharu G.
- The Astrophysical Journal, Vol. 885, Issue 1
Resolving 3D Disk Orientation Using High-resolution Images: New Constraints on Circumgalactic Gas Inflows
journal, December 2019
- Ho, Stephanie H.; Martin, Crystal L.
- The Astrophysical Journal, Vol. 888, Issue 1
Synthetic Gaia Surveys from the FIRE Cosmological Simulations of Milky Way-mass Galaxies
journal, January 2020
- Sanderson, Robyn E.; Wetzel, Andrew; Loebman, Sarah
- The Astrophysical Journal Supplement Series, Vol. 246, Issue 1
Galaxy disc scaling relations: A tight linear galaxy–halo connection challenges abundance matching
journal, September 2019
- Posti, Lorenzo; Marasco, Antonino; Fraternali, Filippo
- Astronomy & Astrophysics, Vol. 629
Morphology and star formation in IllustrisTNG: the build-up of spheroids and discs
journal, June 2019
- Tacchella, Sandro; Diemer, Benedikt; Hernquist, Lars
- Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 4
Dark-ages reionization and galaxy formation simulation – XVII. Sizes, angular momenta, and morphologies of high-redshift galaxies
journal, July 2019
- Marshall, Madeline A.; Mutch, Simon J.; Qin, Yuxiang
- Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 2
Be it therefore resolved: cosmological simulations of dwarf galaxies with 30 solar mass resolution
journal, October 2019
- Wheeler, Coral; Hopkins, Philip F.; Pace, Andrew B.
- Monthly Notices of the Royal Astronomical Society, Vol. 490, Issue 3
Exploring the Very Extended Low-surface-brightness Stellar Populations of the Large Magellanic Cloud with SMASH
journal, March 2019
- Nidever, David L.; Olsen, Knut; Choi, Yumi
- The Astrophysical Journal, Vol. 874, Issue 2
The OSIRIS Lens-amplified Survey (OLAS). I. Dynamical Effects of Stellar Feedback in Low-mass Galaxies at z ∼ 2
journal, July 2019
- Hirtenstein, Jessie; Jones, Tucker; Wang, Xin
- The Astrophysical Journal, Vol. 880, Issue 1
A Closer Look at Bursty Star Formation with L H α and L UV Distributions
journal, August 2019
- Emami, Najmeh; Siana, Brian; Weisz, Daniel R.
- The Astrophysical Journal, Vol. 881, Issue 1
New Horizon: On the Origin of the Stellar Disk and Spheroid of Field Galaxies at z = 0.7
journal, September 2019
- Park, Min-Jung; Yi, Sukyoung K.; Dubois, Yohan
- The Astrophysical Journal, Vol. 883, Issue 1
The Dark Matter Distributions in Low-mass Disk Galaxies. II. The Inner Density Profiles
journal, December 2019
- Relatores, Nicole C.; Newman, Andrew B.; Simon, Joshua D.
- The Astrophysical Journal, Vol. 887, Issue 1
Simulating galaxies in the reionization era with FIRE-2: galaxy scaling relations, stellar mass functions, and luminosity functions
text, January 2018
- Ma, Xiangcheng; Hopkins, Philip F.; Garrison-Kimmel, Shea
- Oxford University Press
Angular momentum evolution of bulge stars in disc galaxies in NIHAO
journal, November 2018
- Wang, Liang; Obreschkow, Danail; Lagos, Claudia del P.
- Monthly Notices of the Royal Astronomical Society, Vol. 482, Issue 4
The origins of the circumgalactic medium in the FIRE simulations
journal, June 2019
- Hafen, Zachary; Faucher-Giguère, Claude-André; Anglés-Alcázar, Daniel
- Monthly Notices of the Royal Astronomical Society, Vol. 488, Issue 1
Formation, vertex deviation, and age of the Milky Way’s bulge: input from a cosmological simulation with a late-forming bar
journal, March 2019
- Debattista, Victor P.; Gonzalez, Oscar A.; Sanderson, Robyn E.
- Monthly Notices of the Royal Astronomical Society, Vol. 485, Issue 4
ZFIRE: 3D Modeling of Rotation, Dispersion, and Angular Momentum of Star-forming Galaxies at z ∼ 2
journal, May 2018
- Alcorn, Leo Y.; Tran, Kim-Vy; Glazebrook, Karl
- The Astrophysical Journal, Vol. 858, Issue 1
The Local Group on FIRE: dwarf galaxy populations across a suite of hydrodynamic simulations
journal, May 2019
- Garrison-Kimmel, Shea; Hopkins, Philip F.; Wetzel, Andrew
- Monthly Notices of the Royal Astronomical Society, Vol. 487, Issue 1
From peculiar morphologies to Hubble-type spirals: the relation between galaxy dynamics and morphology in star-forming galaxies at z ∼ 1.5
journal, December 2019
- Gillman, S.; Tiley, A. L.; Swinbank, A. M.
- Monthly Notices of the Royal Astronomical Society, Vol. 492, Issue 1
Reconciling Observed and Simulated Stellar Halo Masses
journal, December 2018
- Sanderson, Robyn E.; Garrison-Kimmel, Shea; Wetzel, Andrew
- The Astrophysical Journal, Vol. 869, Issue 1
Star formation histories of dwarf galaxies in the FIRE simulations: dependence on mass and Local Group environment
text, January 2019
- Garrison-Kimmel, Shea; Wetzel, Andrew; Hopkins, Philip F.
- Oxford University Press
The connection between mass, environment, and slow rotation in simulated galaxies
journal, February 2018
- Lagos, Claudia del P.; Schaye, Joop; Bahé, Yannick
- Monthly Notices of the Royal Astronomical Society, Vol. 476, Issue 4
Star formation histories of dwarf galaxies in the FIRE simulations: dependence on mass and Local Group environment
journal, September 2019
- Garrison-Kimmel, Shea; Wetzel, Andrew; Hopkins, Philip F.
- Monthly Notices of the Royal Astronomical Society, Vol. 489, Issue 4
On the Origin of Star–Gas Counterrotation in Low-mass Galaxies
journal, June 2019
- Starkenburg, Tjitske K.; Sales, Laura. V.; Genel, Shy
- The Astrophysical Journal, Vol. 878, Issue 2
Simulating galaxies in the reionization era with FIRE-2: galaxy scaling relations, stellar mass functions, and luminosity functions
text, January 2017
- Ma, Xiangcheng; Hopkins, Philip F.; Garrison-Kimmel, Shea
- arXiv
The origin of ultra diffuse galaxies: stellar feedback and quenching
text, January 2017
- Chan, T. K.; Kereš, D.; Wetzel, A.
- arXiv
The star formation rate and stellar content contributions of morphological components in the EAGLE simulations
text, January 2018
- Trayford, James W.; Frenk, Carlos S.; Theuns, Tom
- arXiv
Connecting and dissecting galaxies' angular momenta and neutral gas in a hierarchical universe: cue DARK SAGE
text, January 2018
- Stevens, Adam R. H.; Lagos, Claudia del P.; Obreschkow, Danail
- arXiv
Angular momentum evolution of bulge stars in disc galaxies in NIHAO
text, January 2018
- Wang, Liang; Obreschkow, Danail; Lagos, Claudia del P.
- arXiv
On the origin of star-gas counterrotation in low-mass galaxies
text, January 2019
- Starkenburg, Tjitske K.; Sales, Laura V.; Genel, Shy
- arXiv
Dark and luminous satellites of LMC-mass galaxies in the FIRE simulations
text, January 2019
- Jahn, Ethan D.; Sales, Laura V.; Wetzel, Andrew
- arXiv
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