arXiv:2109.06898v1 [astro-ph.GA] 14 Sep 2021
Gabor - Utopia Chunky Wedge Boots Black - 780.17, The Shoe Horn
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
ORIGINAL UNEDITED MANUSCRIPT
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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
Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤ z < 3 - IOPscience
Rode GABOR Enkellaarsjes 780.1 | Omoda
Synthetic H α maps of galaxies with off-centre bright clumps, marked by... | Download Scientific Diagram
Stellar feedback in a clumpy galaxy at z ∼ 3.4
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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
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
From giant clumps to clouds – I. The impact of gas fraction evolution on the stability of galactic discs
ORIGINAL UNEDITED MANUSCRIPT
Alec OWENS | Research Fellow | Doctor of Philosophy | University College London, London | UCL | Department of Physics and Astronomy
arXiv:1904.04507v3 [astro-ph.GA] 4 Aug 2019
