Results 131 to 140 of about 146 (146)
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Molecular Gas and Star Formation in Galaxies
1997Using the 14m millimeter telescope of the Five College Radio Astronomy Observatory (HPBW=45″), we have observed the CO J=l-0 emission at 1412 positions in 300 galaxies. These observations, which comprise the FCRAO Extragalactic CO Survey, are the most extensive and uniform database on the content and large-scale distribution of molecular gas content in
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Galaxy‐galaxy interactions as triggers of star formation
Astronomische Nachrichten, 2009AbstractGalaxy‐galaxy interactions represent the main physical processes that trigger substantial star formation in galaxies. In order to study the galaxy interactions effects on color and morphology of the galaxies in the fields of two radio galaxies at z ∼ 1, we combined optical‐NIR photometry and HST/WFPC2 morphology data from the Stanford et al ...
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From star formation to galaxy formation
2008Current scenarios for the large-scale structure of the universe lead to rather precise predictions for the structure and evolution of primeval galaxies. These scenarios are reviewed, and models of protogalaxies are described. I discuss the origin of the first stars, and the chemical evolution of galaxies.
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The modelling of feedback in star formation simulations
New Astronomy Reviews, 2015James E Dale
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The insignificance of major mergers in driving star formation at z ≃ 2
Monthly Notices of the Royal Astronomical Society: Letters, 2013Nimish P Hathi +2 more
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Evolution of galaxy stellar masses and star formation rates in the eagle simulations
Monthly Notices of the Royal Astronomical Society, 2015Robert A Crain +2 more
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A unified model for galactic discs: star formation, turbulence driving, and mass transport
Monthly Notices of the Royal Astronomical Society, 2018Blakesley Burkhart +2 more
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