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
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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
Péter Ábrahám's research works | Eötvös Loránd University, Budapest and other places
Template for NKS final reports and guidelines to authors
ALMA 200 pc Resolution Imaging of Smooth Cold Dusty Disks in Typical z ∼ 3 Star-forming Galaxies
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arXiv:1904.04507v3 [astro-ph.GA] 4 Aug 2019
Stellar feedback in a clumpy galaxy at z ∼ 3.4
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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
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
A contribution of star-forming clumps and accreting satellites to the mass assembly of z ∼ 2 galaxies
