FORMATION AND EVOLUTION OF GALAXY DISKS

By Reynier Peletier, K. Ganda, J. Falc'on-Barroso, R. Bacon, M. Cappellari, Roger Davies, P. de Zeeuw, Eric Emsellem, D. Krajnovi'c, H. Kuntschner and 3 more. 2008

149 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/0d70c7bfebf365f2886ebc45e987aa3b02431290

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Citations in the corpus

• Dawes Review 4: Spiral Structures in Disc Galaxies (2014, background): “This may take the form of gravitational instabilities induced by asymmetries in the dark matter profiles of galaxies (Khoperskov et al. 2013), or tidal perturbations from dark matter sub halos (Tutukov & Fedorova 2006; Dubinski et al. 2008; Kazantzidis et al. 2008; Chang & Chakrabarti 2011).”
• INSIDE OUT AND UPSIDE DOWN: TRACING THE ASSEMBLY OF A SIMULATED DISK GALAXY USING MONO-AGE STELLAR POPULATIONS (2013, background): “This general age-velocity relationship (AVR) exists in the MW as well (e.g., Freeman 2008), and it is often explained by older stars having more time to be heated by various perturbing events (e.g., molecular clouds, transient waves, satellites).”
• BULGE n AND B/T IN HIGH-MASS GALAXIES: CONSTRAINTS ON THE ORIGIN OF BULGES IN HIERARCHICAL MODELS (2008, background): “Major mergers are considered as those with stellar mass ratio M1/M2 ≥ 1/4.”
• FORMATION OF MASSIVE GALAXIES AT HIGH REDSHIFT: COLD STREAMS, CLUMPY DISKS, AND COMPACT SPHEROIDS (2009, background): “The spheroids continue to grow according to the standard scenario; bulges develop by slow secular evolution in the disks (Bureau & Athanassoula 2005; Athanassoula 2008), and all spheroids, including today’s giant ellipticals, grow by minor and major mergers.”
• Quasi-linear formulation of MOND (2009, background): “2008), escape speed from a galaxy (Famaey, Bruneton, & Zhao 2007, Wu et al. 2007), galaxy interactions (Tiret & Combes 2007, Nipoti Londrillo & Ciotti 2007a), and collapse (Nipoti, Londrillo & Ciotti 2007b), triaxial models of galactic systems (Wang, Wu, & Zhao 2008, Wu & al.”
• Kinematics and history of the solar neighbourhood revisited (2009, background): “Sellwood (2008) has recently redetermined these ratios and finds σ 1/σ 2 = 1.41 and σ 1/σ 3 = 1.61, both of which are smaller than Fig.”
• MaGICC discs: matching observed galaxy relationships over a wide stellar mass range (2012, background): “This was pointed out in Dutton & Courteau (2008).”
• GALACTOSEISMOLOGY: DISCOVERY OF VERTICAL WAVES IN THE GALACTIC DISK (2012, background): “In addition, Gauthier et al. (2006) and Dubinski et al. (2008) showed that satellites and halo substructure can provoke spiraltype structures in a stellar disk and trigger bar formation.”
• DWARF GALAXY STARBURST STATISTICS IN THE LOCAL VOLUME (2008, methodology): “In Figure 1(c), we plot the Schechter function fits to LFs from two independent data sets that have morphological makeups which should be similar to the 11HUGS sample.”
• Thin, thick and dark discs in ΛCDM (2008, background): “Dubinski et al. (2008) and Gauthier et al. (2006) merge 100 satellites with a simulated M31 galaxy.”