GALAXY STRUCTURE, STELLAR POPULATIONS, AND STAR FORMATION QUENCHING AT 0.6 ≲ <i>z</i> ≲ 1.2. [PDF]
Kim K+5 more
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Molecular tracers of radiative feedback in Orion (OMC-1) Widespread CH<sup>+</sup> (<i>J</i> = 1-0), CO (10-9), HCN (6-5), and HCO<sup>+</sup> (6-5) emission. [PDF]
Goicoechea JR+6 more
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Numerous Old Starburst Galaxies in the Local Universe
Hideaki Mouri, Y. Taniguchi
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Infrared Dust Emission in Starburst Galaxies: Self-Consistent Modeling From the UV to Far Infrared.
K. A. Misselt
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Gravitational-wave localization alone can probe origin of stellar-mass black hole mergers. [PDF]
Bartos I+5 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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Supernova dust destruction in the magnetized turbulent ISM. [PDF]
Kirchschlager F, Mattsson L, Gent FA.
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Dusty starburst galaxies in the early Universe as revealed by gravitational lensing
Nature, 2013In the past decade, our understanding of galaxy evolution has been revolutionized by the discovery that luminous, dusty starburst galaxies were 1,000 times more abundant in the early Universe than at present.
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