The SAMI galaxy survey : understanding observations of large-scale outflows at low redshift with EAGLE simulations
This work presents a study of galactic outflows driven by stellar feedback. We extract main-sequence disc galaxies with stellar mass 10(9) <= M-*/M-circle dot <= 5.7 x 10(10) at redshift z = 0 from the highest resolution cosmological simulation of the Evolution and Assembly of GaLaxies and the...
Published in: | Monthly Notices of the Royal Astronomical Society |
---|---|
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
U.K., Oxford University Press
2018
|
Subjects: | |
Online Access: | https://doi.org/10.1093/mnras/stx2315 https://hdl.handle.net/1959.7/uws:64574 |
id |
ftunivwestsyd:oai:researchdirect.westernsydney.edu.au:uws_64574 |
---|---|
record_format |
openpolar |
spelling |
ftunivwestsyd:oai:researchdirect.westernsydney.edu.au:uws_64574 2023-05-15T18:11:52+02:00 The SAMI galaxy survey : understanding observations of large-scale outflows at low redshift with EAGLE simulations Tescari, E. Cortese, L. Power, C. Wyithe, J. S. B. Ho, I.- T. Crain, R. A. Bland-Hawthorn, J. Croom, S. M. Kewley, L. J. Schaye, J. Bower, R. G. Theuns, T. Schaller, M. Barnes, Luke A. (R19196) Brough, S. Bryant, J. J. Goodwin, M. Gunawardhana, M. L. P. Lawrence, J. S. Leslie, S. K. Lopez-Sanchez, A. R. Lorente, N. P. F. Medling, A. M. Richards, S. N. Sweet, S. M. Tonini, C. 2018 print 18 https://doi.org/10.1093/mnras/stx2315 https://hdl.handle.net/1959.7/uws:64574 eng eng U.K., Oxford University Press Monthly Notices of the Royal Astronomical Society--0035-8711--1365-2966 Vol. 473 Issue. 1 No. pp: 380-397 XXXXXX - Unknown journal article 2018 ftunivwestsyd https://doi.org/10.1093/mnras/stx2315 2022-06-06T22:25:10Z This work presents a study of galactic outflows driven by stellar feedback. We extract main-sequence disc galaxies with stellar mass 10(9) <= M-*/M-circle dot <= 5.7 x 10(10) at redshift z = 0 from the highest resolution cosmological simulation of the Evolution and Assembly of GaLaxies and their Environments (EAGLE) set. Synthetic gas rotation velocity and velocity dispersion (s) maps are created and compared to observations of disc galaxies obtained with the Sydney-AAO (Australian Astronomical Observatory) Multi-object Integral field spectrograph (SAMI), where sigma-values greater than 150 km s(-1) are most naturally explained by bipolar outflows powered by starburst activity. We find that the extension of the simulated edge-on (pixelated) velocity dispersion probability distribution depends on stellar mass and star formation rate surface density (Sigma(SFR)), with low-M*/low-Sigma(SFR) galaxies showing a narrow peak at low sigma (similar to 30 km s(-1)) and more active, high-M-*/high-Sigma(SFR) galaxies reaching sigma > 150 km s(-1). Although supernova-driven galactic winds in the EAGLE simulations may not entrain enough gas with T < 10(5) K compared to observed galaxies, we find that gas temperature is a good proxy for the presence of outflows. There is a direct correlation between the thermal state of the gas and its state of motion as described by the sigma-distribution. The following equivalence relations hold in EAGLE: (i) low-sigma peak double left right arrow disc of the galaxy double left right arrow gas with T < 10(5) K; (ii) high-sigma tail double left right arrow galactic winds double left right arrow gas with T >= 10(5) K. Article in Journal/Newspaper sami University of Western Sydney (UWS): Research Direct Monthly Notices of the Royal Astronomical Society 473 1 380 397 |
institution |
Open Polar |
collection |
University of Western Sydney (UWS): Research Direct |
op_collection_id |
ftunivwestsyd |
language |
English |
topic |
XXXXXX - Unknown |
spellingShingle |
XXXXXX - Unknown Tescari, E. Cortese, L. Power, C. Wyithe, J. S. B. Ho, I.- T. Crain, R. A. Bland-Hawthorn, J. Croom, S. M. Kewley, L. J. Schaye, J. Bower, R. G. Theuns, T. Schaller, M. Barnes, Luke A. (R19196) Brough, S. Bryant, J. J. Goodwin, M. Gunawardhana, M. L. P. Lawrence, J. S. Leslie, S. K. Lopez-Sanchez, A. R. Lorente, N. P. F. Medling, A. M. Richards, S. N. Sweet, S. M. Tonini, C. The SAMI galaxy survey : understanding observations of large-scale outflows at low redshift with EAGLE simulations |
topic_facet |
XXXXXX - Unknown |
description |
This work presents a study of galactic outflows driven by stellar feedback. We extract main-sequence disc galaxies with stellar mass 10(9) <= M-*/M-circle dot <= 5.7 x 10(10) at redshift z = 0 from the highest resolution cosmological simulation of the Evolution and Assembly of GaLaxies and their Environments (EAGLE) set. Synthetic gas rotation velocity and velocity dispersion (s) maps are created and compared to observations of disc galaxies obtained with the Sydney-AAO (Australian Astronomical Observatory) Multi-object Integral field spectrograph (SAMI), where sigma-values greater than 150 km s(-1) are most naturally explained by bipolar outflows powered by starburst activity. We find that the extension of the simulated edge-on (pixelated) velocity dispersion probability distribution depends on stellar mass and star formation rate surface density (Sigma(SFR)), with low-M*/low-Sigma(SFR) galaxies showing a narrow peak at low sigma (similar to 30 km s(-1)) and more active, high-M-*/high-Sigma(SFR) galaxies reaching sigma > 150 km s(-1). Although supernova-driven galactic winds in the EAGLE simulations may not entrain enough gas with T < 10(5) K compared to observed galaxies, we find that gas temperature is a good proxy for the presence of outflows. There is a direct correlation between the thermal state of the gas and its state of motion as described by the sigma-distribution. The following equivalence relations hold in EAGLE: (i) low-sigma peak double left right arrow disc of the galaxy double left right arrow gas with T < 10(5) K; (ii) high-sigma tail double left right arrow galactic winds double left right arrow gas with T >= 10(5) K. |
format |
Article in Journal/Newspaper |
author |
Tescari, E. Cortese, L. Power, C. Wyithe, J. S. B. Ho, I.- T. Crain, R. A. Bland-Hawthorn, J. Croom, S. M. Kewley, L. J. Schaye, J. Bower, R. G. Theuns, T. Schaller, M. Barnes, Luke A. (R19196) Brough, S. Bryant, J. J. Goodwin, M. Gunawardhana, M. L. P. Lawrence, J. S. Leslie, S. K. Lopez-Sanchez, A. R. Lorente, N. P. F. Medling, A. M. Richards, S. N. Sweet, S. M. Tonini, C. |
author_facet |
Tescari, E. Cortese, L. Power, C. Wyithe, J. S. B. Ho, I.- T. Crain, R. A. Bland-Hawthorn, J. Croom, S. M. Kewley, L. J. Schaye, J. Bower, R. G. Theuns, T. Schaller, M. Barnes, Luke A. (R19196) Brough, S. Bryant, J. J. Goodwin, M. Gunawardhana, M. L. P. Lawrence, J. S. Leslie, S. K. Lopez-Sanchez, A. R. Lorente, N. P. F. Medling, A. M. Richards, S. N. Sweet, S. M. Tonini, C. |
author_sort |
Tescari, E. |
title |
The SAMI galaxy survey : understanding observations of large-scale outflows at low redshift with EAGLE simulations |
title_short |
The SAMI galaxy survey : understanding observations of large-scale outflows at low redshift with EAGLE simulations |
title_full |
The SAMI galaxy survey : understanding observations of large-scale outflows at low redshift with EAGLE simulations |
title_fullStr |
The SAMI galaxy survey : understanding observations of large-scale outflows at low redshift with EAGLE simulations |
title_full_unstemmed |
The SAMI galaxy survey : understanding observations of large-scale outflows at low redshift with EAGLE simulations |
title_sort |
sami galaxy survey : understanding observations of large-scale outflows at low redshift with eagle simulations |
publisher |
U.K., Oxford University Press |
publishDate |
2018 |
url |
https://doi.org/10.1093/mnras/stx2315 https://hdl.handle.net/1959.7/uws:64574 |
genre |
sami |
genre_facet |
sami |
op_relation |
Monthly Notices of the Royal Astronomical Society--0035-8711--1365-2966 Vol. 473 Issue. 1 No. pp: 380-397 |
op_doi |
https://doi.org/10.1093/mnras/stx2315 |
container_title |
Monthly Notices of the Royal Astronomical Society |
container_volume |
473 |
container_issue |
1 |
container_start_page |
380 |
op_container_end_page |
397 |
_version_ |
1766184482118828032 |