Galaxy formation through hierarchical clustering

Keywords

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

References

No references recorded for this paper.

Cited by

• Magnetic Field Evolution in Isolated and Interacting Spiral GalaxiesHanna Kotarba — 2011
• Tópicos sobre formação e estrutura da via lácteaLiliane Lewis Xerxenevsky — 2008
• Morphological evolution of galaxies over the last 8 billion yearsM. Pannella — 2007
• Connecting cosmological simulations to the real worldCarlos S. Frenk — 2003
• Analytical Modelling of Galaxy FormationAlberto Manrique, Eduard Salvador-Solé — 1998
• An Analytical Model of Galaxy FormationEduard Salvador-Solé, Alberto Manrique, A. Raig — 2001
• The surface brightness distribution of Virgo cluster galaxiesM. McDonald — 2007
• The Quest for ProtogalaxiesS. G. Djorgovski — 1996
• The impact of active galactic nuclei on cooling flowsC. D. Vecchia — 2005
• Measuring the star formation rate density from CNOC2Richard Whitaker — 2006
• A numerical study of galaxy mass density profilesK. Foyle — 2007
• Modélisation de l'émission Lyman-alpha dans les galaxies à grand décalage spectral et simulations cosmologiquesT. Garel — 2011
• Interactions of Dark and Baryonic Matter in Dwarf GalaxiesDavid R. Cole — 2012
• NIHAO III: the constant disc gas mass conspiracyGregory S. Stinson, Aaron A. Dutton, L. Wang — 2015
• ZEPLIN-III direct dark matter search : final results and measurements in support of next generation instrumentsL. Reichhart — 2013
• Co-evolution of galaxies and black holesM. Hirschmann — 2011
• Galaxies in a simulated ΛCDM Universe – I. Cold mode and hot coresDušan Kereš, Neal Katz, Mark A. Fardal — 2008
• Gusty, gaseous flows of FIRE: Galactic winds in cosmological simulations with explicit stellar feedbackAlexander L. Muratov, Dušan Kereš, Claude‐André Faucher‐Giguère — 2015
• THE STATE OF THE COLD DARK MATTER MODELS ON GALACTIC AND SUBGALACTIC SCALESARGYRO TASITSIOMI — 2002
• The cosmological mass functionA. Del Popolo, I. S. Yesilyurt — 2006

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