Synthetic H α maps of galaxies with off-centre bright clumps, marked by... | Download Scientific Diagram
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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
From giant clumps to clouds – I. The impact of gas fraction evolution on the stability of galactic discs
DIFFERENT STAR FORMATION LAWS FOR DISKS VERSUS STARBURSTS AT LOW AND HIGH REDSHIFTS - IOPscience
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Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ⩽ z < 3
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
ALMA 200 pc Resolution Imaging of Smooth Cold Dusty Disks in Typical z ∼ 3 Star-forming Galaxies
Template for NKS final reports and guidelines to authors
Clumpy Galaxies in CANDELS. II. Physical Properties of UV-bright Clumps at 0.5 ≤ z < 3 - IOPscience
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arXiv:2109.06898v1 [astro-ph.GA] 14 Sep 2021
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