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Stellar feedback in a clumpy galaxy at z ∼ 3.4
From giant clumps to clouds – I. The impact of gas fraction evolution on the stability of galactic discs
Alec OWENS | Research Fellow | Doctor of Philosophy | University College London, London | UCL | Department of Physics and Astronomy
arXiv:2109.06898v1 [astro-ph.GA] 14 Sep 2021
From giant clumps to clouds – I. The impact of gas fraction evolution on the stability of galactic discs
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Synthetic H α maps of galaxies with off-centre bright clumps, marked by... | Download Scientific Diagram
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
