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ALMA resolves the properties of star-forming regions in a dense gas disk at z ∼ 3

Swinbank, A.M.; Dye, S.; Nightingale, J.W.; Furlanetto, C.; Smail, Ian; Cooray, A.; Dannerbauer, H.; Dunne, L.; Eales, S.; Gavazzi, R.; Hunter, T.; Ivison, R.J.; Negrello, M.; Oteo-Gomez, I.; Smit, R.; Werf, P. van der; Vlahakis, C.

Authors

A.M. Swinbank

SIMON DYE Simon.Dye@nottingham.ac.uk
Associate Professor

J.W. Nightingale

C. Furlanetto

Ian Smail

A. Cooray

H. Dannerbauer

L. Dunne

S. Eales

R. Gavazzi

T. Hunter

R.J. Ivison

M. Negrello

I. Oteo-Gomez

R. Smit

P. van der Werf

C. Vlahakis



Abstract

We exploit long baseline ALMA submillimeter observations of the lensed star-forming galaxy SDP 81 at z = 3.042 to investigate the properties of the interstellar medium (ISM) on scales of 50–100 pc. The kinematics of the 12CO gas within this system are well described by a rotationally supported disk with an inclination-corrected rotation speed, = 320 ± 20 km s−1, and a dynamical mass of = (3.5 ± 1.0)× 1010 within a radius of 1.5 kpc. The disk is gas-rich and unstable, with a Toomre parameter, Q = 0.30 ± 0.10, and so into star-forming regions with Jeans length 130 pc. We identify five star-forming regions within the ISM on these scales and show that their scaling relations between luminosity, line widths, and sizes are significantly offset from those typical of molecular clouds in local galaxies (Larson's relations). These offsets are likely to be caused by the high external hydrostatic pressure for the ISM, / × 107 K cm−3, which is ~104× higher than the typical ISM pressure in the Milky Way. The physical conditions of the star-forming ISM and giant molecular clouds appear to be similar to those found in the densest environments in the local universe, such as those in the Galactic center.

Citation

Swinbank, A., Dye, S., Nightingale, J., Furlanetto, C., Smail, I., Cooray, A., …Vlahakis, C. (2015). ALMA resolves the properties of star-forming regions in a dense gas disk at z ∼ 3. Astrophysical Journal Letters, 806(1), https://doi.org/10.1088/2041-8205/806/1/L17

Journal Article Type Article
Acceptance Date May 18, 2015
Publication Date Jun 9, 2015
Deposit Date Apr 27, 2017
Publicly Available Date Apr 27, 2017
Journal Astrophysical Journal Letters
Print ISSN 2041-8205
Electronic ISSN 2041-8213
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 806
Issue 1
Article Number L17
DOI https://doi.org/10.1088/2041-8205/806/1/L17
Keywords galaxies: evolution; galaxies: high-redshift; galaxies: starburst
Public URL http://eprints.nottingham.ac.uk/id/eprint/42359
Publisher URL http://iopscience.iop.org/article/10.1088/2041-8205/806/1/L17/meta
Copyright Statement Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf

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Copyright Statement
Copyright information regarding this work can be found at the following address: http://eprints.nottingham.ac.uk/end_user_agreement.pdf





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