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A contribution of star-forming clumps and accreting satellites to the mass assembly of z ∼ 2 galaxies
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Rode GABOR Enkellaarsjes 780.1 | Omoda
ALMA 200 pc Resolution Imaging of Smooth Cold Dusty Disks in Typical z ∼ 3 Star-forming Galaxies
From giant clumps to clouds – I. The impact of gas fraction evolution on the stability of galactic discs
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arXiv:1904.04507v3 [astro-ph.GA] 4 Aug 2019
A contribution of star-forming clumps and accreting satellites to the mass assembly of z ∼ 2 galaxies
Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤ z < 3 - IOPscience
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From giant clumps to clouds – I. The impact of gas fraction evolution on the stability of galactic discs
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arXiv:1904.04507v3 [astro-ph.GA] 4 Aug 2019
A contribution of star-forming clumps and accreting satellites to the mass assembly of z ∼ 2 galaxies
Alec OWENS | Research Fellow | Doctor of Philosophy | University College London, London | UCL | Department of Physics and Astronomy
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
Rode GABOR Enkellaarsjes 780.1 | Omoda
Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ⩽ z < 3