From giant clumps to clouds – I. The impact of gas fraction evolution on the stability of galactic discs
Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤ z < 3 - IOPscience
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arXiv:1904.04507v3 [astro-ph.GA] 4 Aug 2019
DIFFERENT STAR FORMATION LAWS FOR DISKS VERSUS STARBURSTS AT LOW AND HIGH REDSHIFTS - IOPscience
arXiv:2109.06898v1 [astro-ph.GA] 14 Sep 2021
A contribution of star-forming clumps and accreting satellites to the mass assembly of z ∼ 2 galaxies
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A contribution of star-forming clumps and accreting satellites to the mass assembly of z ∼ 2 galaxies
From giant clumps to clouds – I. The impact of gas fraction evolution on the stability of galactic discs
From giant clumps to clouds – I. The impact of gas fraction evolution on the stability of galactic discs
Template for NKS final reports and guidelines to authors
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PDF) The chronostratigraphy of the Haua Fteah cave (Cyrenaica, northeast Libya) | Tim Reynolds - Academia.edu
From giant clumps to clouds – I. The impact of gas fraction evolution on the stability of galactic discs
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ALMA 200 pc Resolution Imaging of Smooth Cold Dusty Disks in Typical z ∼ 3 Star-forming Galaxies
arXiv:2109.06898v1 [astro-ph.GA] 14 Sep 2021
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Alec OWENS | Research Fellow | Doctor of Philosophy | University College London, London | UCL | Department of Physics and Astronomy
