The Role of Dust in the Early Universe I : Protogalaxy Evolution

Keywords

Physics, Star formation, Astrophysics, Galaxy, Galaxy formation and evolution

References

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• Dust Destruction in the High-Velocity Shocks Driven by Supernovae in the Early UniverseTakaya Nozawa, Takashi Kozasa, Asao Habe — 2006
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Cited by

• THE ORIGIN OF DUST EXTINCTION CURVES WITH OR WITHOUT THE 2175 Å BUMP IN GALAXIES: THE CASE OF THE MAGELLANIC CLOUDSKenji Bekki, Hiroyuki Hirashita, Takuji Tsujimoto — 2015
• The role of dust in models of population synthesisL. P. Cassará, L. Piovan, A. Weiß — 2013
• Synthesized grain size distribution in the interstellar mediumHiroyuki Hirashita, Takaya Nozawa — 2012
• Evolution of dust content in galaxies probed by gamma-ray burst afterglowsTzu-Ming Kuo, Hiroyuki Hirashita, Tayyaba Zafar — 2013
• Dense molecular cloud cores as a source of micrometer-sized grains in galaxiesHiroyuki Hirashita, Ryosuke S. Asano, Takaya Nozawa — 2014
• Dust formation history of galaxies: A critical role of metallicity* for the dust mass growth by accreting materials in the interstellar mediumRyosuke S. Asano, Tsutomu T. Takeuchi, Hiroyuki Hirashita — 2012
• Dust properties of Lyman-break galaxies in cosmological simulationsHidenobu Yajima, Kentaro Nagamine, Robert M. Thompson — 2013
• Chemical complexity in astrophysical simulations: optimization and reduction techniquesTommaso Grassi, S. Bovino, D. R. G. Schleicher — 2012
• What determines the grain size distribution in galaxiesRyosuke S. Asano, Tsutomu T. Takeuchi, Hiroyuki Hirashita — 2013
• Evolution of thermally pulsing asymptotic giant branch stars - III. Dust production at supersolar metallicitiesA. Nanni, A. Bressan, Paola Marigo — 2013
• FORMATION OF SiC GRAINS IN PULSATION-ENHANCED DUST-DRIVEN WIND AROUND CARBON-RICH ASYMPTOTIC GIANT BRANCH STARSYuki Yasuda, Takashi Kozasa — 2011
• Carbon cations and silicon atoms in the ISM: modelling their charge exchange reactionMauro Satta, Tommaso Grassi, F. A. Gianturco — 2012
• Modelling galaxy spectra in presence of interstellar dust – III. From nearby galaxies to the distant UniverseL. P. Cassará, L. Piovan, C. Chiosi — 2014
• Evolution of grain size distribution in high-redshift dusty quasars: integrating large amounts of dust and unusual extinction curvesTakaya Nozawa, Ryosuke S. Asano, Hiroyuki Hirashita — 2014
• The equilibrium view on dust and metals in galaxies: Galactic outflows drive low dust-to-metal ratios in dwarf galaxiesRobert Feldmann — 2014
• Reducing Si population in the ISM by charge exchange collisions with He + : a quantum modelling of the processMauro Satta, Tommaso Grassi, F. A. Gianturco — 2013
• Effects of grain growth mechanisms on the extinction curve and the metal depletion in the interstellar mediumHiroyuki Hirashita, Н. В. Вощинников — 2013
• Coevolution of dust, gas and stars in galaxies – I. Spatial distributions and scaling-relations of dust and molecular hydrogenKenji Bekki — 2013
• Dust Formation in Milky Way-like GalaxiesR. McKinnon, Paul Torrey, Mark Vogelsberger — 2015
• Evolution of extinction curves in galaxiesRyosuke S. Asano, Tsutomu T. Takeuchi, Hiroyuki Hirashita — 2014

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• Formation and Processing of Interstellar Dust.Takashi Onaka — 1991
• Astrophysical dust grains in stars, the interstellar medium, and the solar systemR. D. Gehrz — 1991
• Ashes to ashes, dust to dustD. A. Williams — 2000
• Smoking Quasars: A New Source for Cosmic DustM. Elvis, M. Marengo, Margarita Karovska — 2002
• Infrared emission by dust grains near variable primary sources. II - A model for infrared novaeM. F. Bode, A. Evans — 1980