A long-duration gamma-ray burst of dynamical origin from the nucleus of an ancient galaxy
Levan A +29 more
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First submillimeter lights from Dome A: Tracing the carbon cycle in the feedback of massive stars. [PDF]
Gong Y +40 more
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Achieving GPT-4o level performance in astronomy with a specialized 8B-parameter large language model. [PDF]
de Haan T +8 more
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Computational approaches to modeling dynamos in galaxies. [PDF]
Korpi-Lagg MJ, Mac Low MM, Gent FA.
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Multiscale Perspectives on Solid-Phase Astrochemistry: Laboratory, Computation, and Open Questions. [PDF]
Dickers MD +3 more
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Potential impact of the Sagittarius dwarf galaxy on the formation of young O-rich stars. [PDF]
Sun T +12 more
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Primordial Rotating Disk Composed of ≥15 Star Forming Clumps at Cosmic Dawn
Fujimoto S +45 more
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Extended hot dust emission around the earliest massive quiescent galaxy
Ji Z +16 more
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The Evolution of the Cold Interstellar Medium in Galaxies Following a Starburst★ [PDF]
VW and KR acknowledge support from the European Research Council Starting Grant SEDmorph (P.I. VW).We present the evolution of dust and molecular gas properties in a sample of 11 z ˜ 0.03 starburst to post-starburst (PSB) galaxies selected to span an age
Kate Rowlands +2 more
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Starburst galaxies – An observer’s view
Astrophysics and Space Science, 2004Starbursts are the most efficient producers of metals in the Universe at low redshifts. They produce enough energy to drive outflows of material from their disks. This makes them important objects to study in order to understand the chemical evolution not only of the interstellar medium (ISM) in the starburst galaxies themselves, but also of the ...
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