Connecting and dissecting galaxies' angular momenta and neutral gas in a hierarchical universe: Cue DARK SAGE

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Abstract

We explore the connection between the atomic gas fraction, fatm, and 'global disc stability' parameter, q, of galaxies within a fully cosmological context by examining galaxies in the DARK SAGE semi-analytic model. The q parameter is determined by the ratio of disc specific angular momentum to mass, i.e. q ∝ jdisc/mdisc. DARK SAGE is well suited to our study, as it includes the numerical evolution of one-dimensional disc structure, making both jdisc and q predicted quantities. We show that DARK SAGE produces a clear correlation between gas fraction and jdisc at fixed disc mass, in line with recent results from observations and hydrodynamic simulations. This translates to a tight q-fatm sequence for star-forming central galaxies, which closely tracks the analytic prediction of Obreschkow et al. The scatter in this sequence is driven by the probability distribution function of mass as a function of j (PDF of j) within discs, specifically where it peaks. We find that halo mass is primarily responsible for the peak location of the PDF of j, at least for low values of q. Two main mechanisms of equal significance are then identified for disconnecting fatm from q. Mergers in the model can trigger quasar winds, with the potential to blow out most of the gas disc, while leaving the stellar disc relatively unharmed. Ram-pressure stripping of satellite galaxies has a similar effect, where fatm can drop drastically with only a minimal effect to q. We highlight challenges associated with following these predictions up with observations.

Original languageEnglish
Pages (from-to)5543-5559
Number of pages17
JournalMonthly Notices of the Royal Astronomical Society
Volume481
Issue number4
DOIs
Publication statusPublished - 1 Dec 2018

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neutral gases
cues
angular momentum
universe
galaxies
gases
gas
prediction
merger
hydrodynamics
ram
monatomic gases
probability distribution functions
predictions
stripping
quasars
halos
simulation
actuators
stars

Cite this

@article{273528bb344a4b38a9929711ced11b56,
title = "Connecting and dissecting galaxies' angular momenta and neutral gas in a hierarchical universe: Cue DARK SAGE",
abstract = "We explore the connection between the atomic gas fraction, fatm, and 'global disc stability' parameter, q, of galaxies within a fully cosmological context by examining galaxies in the DARK SAGE semi-analytic model. The q parameter is determined by the ratio of disc specific angular momentum to mass, i.e. q ∝ jdisc/mdisc. DARK SAGE is well suited to our study, as it includes the numerical evolution of one-dimensional disc structure, making both jdisc and q predicted quantities. We show that DARK SAGE produces a clear correlation between gas fraction and jdisc at fixed disc mass, in line with recent results from observations and hydrodynamic simulations. This translates to a tight q-fatm sequence for star-forming central galaxies, which closely tracks the analytic prediction of Obreschkow et al. The scatter in this sequence is driven by the probability distribution function of mass as a function of j (PDF of j) within discs, specifically where it peaks. We find that halo mass is primarily responsible for the peak location of the PDF of j, at least for low values of q. Two main mechanisms of equal significance are then identified for disconnecting fatm from q. Mergers in the model can trigger quasar winds, with the potential to blow out most of the gas disc, while leaving the stellar disc relatively unharmed. Ram-pressure stripping of satellite galaxies has a similar effect, where fatm can drop drastically with only a minimal effect to q. We highlight challenges associated with following these predictions up with observations.",
keywords = "Galaxies: evolution, Galaxies: haloes, Galaxies: interactions, Galaxies: ISM, Galaxies: star formation",
author = "Stevens, {Adam R.H.} and Lagos, {Claudia del P.} and Danail Obreschkow and Manodeep Sinha",
year = "2018",
month = "12",
day = "1",
doi = "10.1093/MNRAS/STY2650",
language = "English",
volume = "481",
pages = "5543--5559",
journal = "Monthly Notices of the Royal Astronomical Society",
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TY - JOUR

T1 - Connecting and dissecting galaxies' angular momenta and neutral gas in a hierarchical universe

T2 - Cue DARK SAGE

AU - Stevens, Adam R.H.

AU - Lagos, Claudia del P.

AU - Obreschkow, Danail

AU - Sinha, Manodeep

PY - 2018/12/1

Y1 - 2018/12/1

N2 - We explore the connection between the atomic gas fraction, fatm, and 'global disc stability' parameter, q, of galaxies within a fully cosmological context by examining galaxies in the DARK SAGE semi-analytic model. The q parameter is determined by the ratio of disc specific angular momentum to mass, i.e. q ∝ jdisc/mdisc. DARK SAGE is well suited to our study, as it includes the numerical evolution of one-dimensional disc structure, making both jdisc and q predicted quantities. We show that DARK SAGE produces a clear correlation between gas fraction and jdisc at fixed disc mass, in line with recent results from observations and hydrodynamic simulations. This translates to a tight q-fatm sequence for star-forming central galaxies, which closely tracks the analytic prediction of Obreschkow et al. The scatter in this sequence is driven by the probability distribution function of mass as a function of j (PDF of j) within discs, specifically where it peaks. We find that halo mass is primarily responsible for the peak location of the PDF of j, at least for low values of q. Two main mechanisms of equal significance are then identified for disconnecting fatm from q. Mergers in the model can trigger quasar winds, with the potential to blow out most of the gas disc, while leaving the stellar disc relatively unharmed. Ram-pressure stripping of satellite galaxies has a similar effect, where fatm can drop drastically with only a minimal effect to q. We highlight challenges associated with following these predictions up with observations.

AB - We explore the connection between the atomic gas fraction, fatm, and 'global disc stability' parameter, q, of galaxies within a fully cosmological context by examining galaxies in the DARK SAGE semi-analytic model. The q parameter is determined by the ratio of disc specific angular momentum to mass, i.e. q ∝ jdisc/mdisc. DARK SAGE is well suited to our study, as it includes the numerical evolution of one-dimensional disc structure, making both jdisc and q predicted quantities. We show that DARK SAGE produces a clear correlation between gas fraction and jdisc at fixed disc mass, in line with recent results from observations and hydrodynamic simulations. This translates to a tight q-fatm sequence for star-forming central galaxies, which closely tracks the analytic prediction of Obreschkow et al. The scatter in this sequence is driven by the probability distribution function of mass as a function of j (PDF of j) within discs, specifically where it peaks. We find that halo mass is primarily responsible for the peak location of the PDF of j, at least for low values of q. Two main mechanisms of equal significance are then identified for disconnecting fatm from q. Mergers in the model can trigger quasar winds, with the potential to blow out most of the gas disc, while leaving the stellar disc relatively unharmed. Ram-pressure stripping of satellite galaxies has a similar effect, where fatm can drop drastically with only a minimal effect to q. We highlight challenges associated with following these predictions up with observations.

KW - Galaxies: evolution

KW - Galaxies: haloes

KW - Galaxies: interactions

KW - Galaxies: ISM

KW - Galaxies: star formation

UR - http://www.scopus.com/inward/record.url?scp=85057597264&partnerID=8YFLogxK

U2 - 10.1093/MNRAS/STY2650

DO - 10.1093/MNRAS/STY2650

M3 - Article

VL - 481

SP - 5543

EP - 5559

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 4

ER -