Testing star formation laws in a starburst galaxy at redshift 3 resolved with ALMA
Using high-resolution (sub-kiloparsec scale) data obtained by ALMA, we analyse the star formation rate (SFR), gas content, and kinematics in SDP 81, a gravitationally lensed starburst galaxy at redshift 3. We estimate the SFR surface density (ΣSFR) in the brightest clump of this galaxy to be 357+135...
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Oxford University Press
2018
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| Online Access: | https://eprints.nottingham.ac.uk/52377/ |
| _version_ | 1848798711742726144 |
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| author | Sharda, P. Federrath, C. da Cunha, E. Swinbank, A.M. Dye, S. |
| author_facet | Sharda, P. Federrath, C. da Cunha, E. Swinbank, A.M. Dye, S. |
| author_sort | Sharda, P. |
| building | Nottingham Research Data Repository |
| collection | Online Access |
| description | Using high-resolution (sub-kiloparsec scale) data obtained by ALMA, we analyse the star formation rate (SFR), gas content, and kinematics in SDP 81, a gravitationally lensed starburst galaxy at redshift 3. We estimate the SFR surface density (ΣSFR) in the brightest clump of this galaxy to be 357+135−85M⊙yr−1kpc−2, over an area of 0.07 ± 0.02 kpc2. Using the intensity-weighted velocity of CO (5–4), we measure the turbulent velocity dispersion in the plane of the sky and find σv, turb = 37 ± 5 km s−1 for the clump, in good agreement with previous estimates along the line of sight. Our measurements of the gas surface density, freefall time, and turbulent Mach number allow us to compare the theoretical SFR from various star formation models with that observed, revealing that the role of turbulence is crucial to explaining the observed SFR in this clump. While the Kennicutt–Schmidt (KS) relation predicts an SFR surface density of ΣSFR, KS = 52 ± 17 M⊙ yr−1 kpc−2, the single-freefall model by Krumholz, Dekel, and McKee (KDM) predicts ΣSFR, KDM = 106 ± 37 M⊙ yr−1 kpc−2. In contrast, the multifreefall (turbulence) model by Salim, Federrath, and Kewley (SFK) gives ΣSFR,SFK=491+139−194M⊙yr−1kpc−2. Although the SFK relation overestimates the SFR in this clump (possibly due to the negligence of magnetic fields), it provides the best prediction among the available models. Finally, we compare the star formation and gas properties of this galaxy to local star-forming regions and find that the SFK relation provides the best estimates of SFR in both local and high-redshift galaxies. |
| first_indexed | 2025-11-14T20:24:07Z |
| format | Article |
| id | nottingham-52377 |
| institution | University of Nottingham Malaysia Campus |
| institution_category | Local University |
| last_indexed | 2025-11-14T20:24:07Z |
| publishDate | 2018 |
| publisher | Oxford University Press |
| recordtype | eprints |
| repository_type | Digital Repository |
| spelling | nottingham-523772020-05-04T19:50:42Z https://eprints.nottingham.ac.uk/52377/ Testing star formation laws in a starburst galaxy at redshift 3 resolved with ALMA Sharda, P. Federrath, C. da Cunha, E. Swinbank, A.M. Dye, S. Using high-resolution (sub-kiloparsec scale) data obtained by ALMA, we analyse the star formation rate (SFR), gas content, and kinematics in SDP 81, a gravitationally lensed starburst galaxy at redshift 3. We estimate the SFR surface density (ΣSFR) in the brightest clump of this galaxy to be 357+135−85M⊙yr−1kpc−2, over an area of 0.07 ± 0.02 kpc2. Using the intensity-weighted velocity of CO (5–4), we measure the turbulent velocity dispersion in the plane of the sky and find σv, turb = 37 ± 5 km s−1 for the clump, in good agreement with previous estimates along the line of sight. Our measurements of the gas surface density, freefall time, and turbulent Mach number allow us to compare the theoretical SFR from various star formation models with that observed, revealing that the role of turbulence is crucial to explaining the observed SFR in this clump. While the Kennicutt–Schmidt (KS) relation predicts an SFR surface density of ΣSFR, KS = 52 ± 17 M⊙ yr−1 kpc−2, the single-freefall model by Krumholz, Dekel, and McKee (KDM) predicts ΣSFR, KDM = 106 ± 37 M⊙ yr−1 kpc−2. In contrast, the multifreefall (turbulence) model by Salim, Federrath, and Kewley (SFK) gives ΣSFR,SFK=491+139−194M⊙yr−1kpc−2. Although the SFK relation overestimates the SFR in this clump (possibly due to the negligence of magnetic fields), it provides the best prediction among the available models. Finally, we compare the star formation and gas properties of this galaxy to local star-forming regions and find that the SFK relation provides the best estimates of SFR in both local and high-redshift galaxies. Oxford University Press 2018-07 Article PeerReviewed Sharda, P., Federrath, C., da Cunha, E., Swinbank, A.M. and Dye, S. (2018) Testing star formation laws in a starburst galaxy at redshift 3 resolved with ALMA. Monthly Notices of the Royal Astronomical Society, 477 (4). pp. 4380-4390. ISSN 1365-2966 Turbulence Stars: formation galaxies: high-redshift galaxies: starburst Galaxy: kinematics and dynamics Submillimetre: galaxies https://academic.oup.com/mnras/article/477/4/4380/4964761 doi:10.1093/mnras/sty886 doi:10.1093/mnras/sty886 |
| spellingShingle | Turbulence Stars: formation galaxies: high-redshift galaxies: starburst Galaxy: kinematics and dynamics Submillimetre: galaxies Sharda, P. Federrath, C. da Cunha, E. Swinbank, A.M. Dye, S. Testing star formation laws in a starburst galaxy at redshift 3 resolved with ALMA |
| title | Testing star formation laws in a starburst galaxy at redshift 3 resolved with ALMA |
| title_full | Testing star formation laws in a starburst galaxy at redshift 3 resolved with ALMA |
| title_fullStr | Testing star formation laws in a starburst galaxy at redshift 3 resolved with ALMA |
| title_full_unstemmed | Testing star formation laws in a starburst galaxy at redshift 3 resolved with ALMA |
| title_short | Testing star formation laws in a starburst galaxy at redshift 3 resolved with ALMA |
| title_sort | testing star formation laws in a starburst galaxy at redshift 3 resolved with alma |
| topic | Turbulence Stars: formation galaxies: high-redshift galaxies: starburst Galaxy: kinematics and dynamics Submillimetre: galaxies |
| url | https://eprints.nottingham.ac.uk/52377/ https://eprints.nottingham.ac.uk/52377/ https://eprints.nottingham.ac.uk/52377/ |