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Galaxy Formation Theory [PDF]
Physics Reports, 2010 We review the current theory of how galaxies form within the cosmological
framework provided by the cold dark matter paradigm for structure formation.
Beginning with the pre-galactic evolution of baryonic material we describe the
analytical and numerical Abadi, Abadi, Abel, Abel, Abel, Abraham, Agertz, Ahn, Allen, Andrew J. Benson, Angus, Arad, Arons, Athanassoula, Athanassoula, Aubert, Bahcall, Bahcall, Banerjee, Bardeen, Barnes, Barnes, Barnes, Baugh, Baugh, Baugh, Baugh, Baugh, Baugh, Baugh, Baugh, Begelman, Begelman, Bell, Belokurov, Belokurov, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Berezinsky, Berti, Bertin, Bertone, Bertschinger, Bertschinger, Bett, Binney, Binney, Birnboim, Birzan, Blaizot, Blaizot, Blaizot, Blanchet, Bland-Hawthorn, Blandford, Blandford, Blumenthal, Blumenthal, Bode, Boehm, Bond, Bondi, Booth, Borgani, Bournaud, Bournaud, Bower, Bower, Bower, Bower, Boylan-Kolchin, Boyle, Bromm, Bromm, Brook, Brook, Brooks, Bruzual, Brüggen, Brüggen, Bullock, Bullock, Bullock, Bullock, Cardone, Cattaneo, Cazaux, Chabrier, Chakrabarti, Chandrasekhar, Chary, Chiu, Christodoulou, Christodoulou, Ciardi, Ciardi, Ciotti, Clarke, Clarke, Cole, Cole, Cole, Cole, Cole, Cole, Cole, Colín, Conroy, Conroy, Conroy, Cooray, Covington, Cox, Cox, Crain, Croton, Croton, Davis, Davé, de Vaucouleurs, Dekel, Devriendt, Devriendt, Diaferio, Dolag, Dotter, Dove, Draine, Dunkley, Dutton, Dutton, Edgar, Efstathiou, Efstathiou, Efstathiou, Einasto, Eisenstein, Eke, Eke, El-Zant, Elahi, Fakhouri, Fakhouri, Fall, Fan, Fardal, Favata, Federrath, Ferland, Ferrara, Ferrarese, Ferrarese, Field, Finlator, Firmani, Fitchett, Font, Font, Font, Font, Fontanot, Fontanot, François, Freeman, Frenk, Frenk, Frenk, Friedli, Fryxell, Galli, Gao, Gao, Gebhardt, Gebhardt, Glover, Gnat, Gnedin, Gnedin, Gnedin, Gnedin, Gnedin, Gnedin, Gnedin, Gnedin, Goerdt, Goldreich, Gonçalves, Gould, Governato, Governato, Governato, Granato, Greif, Guiderdoni, Gunn, Gunn, Guo, Gustafsson, Haardt, Hahn, Hamilton, Harris, Hatton, Heitmann, Helly, Helly, Henriques, Hernquist, Hollenbach, Hoyle, Hubble, Jenkins, Jenkins, Jiang, Jing, Jog, Johnston, Jonsson, Jubelgas, Kampakoglou, Kant, Katz, Katz, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kaufmann, Kay, Kazantzidis, Kennicutt, Kennicutt, Kereš, Kereš, King, King, King, Klypin, Klypin, Klypin, Kobayashi, Komatsu, Komissarov, Kormendy, Kormendy, Kormendy, Kowalski, Kravtsov, Kravtsov, Kravtsov, Kriek, Kroupa, Krumholz, Kuhlen, Kuijken, Lacey, Lacey, Lacey, Lacey, Lanzoni, Larson, Laursen, Law, Lawlor, Lee, Lemson, Li, Li, Libeskind, Lin, Lin, Lintott, Lotz, Lotz, Lucia, Lucia, Lucia, Lynden-Bell, Lynden-Bell, Machida, Madau, Madau, Madau, Magorrian, Malbon, Maller, Maller, Maller, Maller, Mandelbaum, Mao, Maraston, Marigo, Marri, Martin, Martínez-Serrano, Mastropietro, Mastropietro, Mateo, Matteo, Matteo, Matteo, Matteucci, Matteucci, Mayer, Mayer, McCarthy, McCarthy, McDowell, McKee, McKee, Meier, Meier, Meiksin, Merritt, Merritt, Milosavljevic, Milosavljevic, Minchev, Miranda, Mo, Monaco, Monaco, Monaco, Moore, Moore, Moore, Moore, Moore, Murali, Murali, Murali, Murray, Nagashima, Nagashima, Narayan, Narayanan, Narlikar, Navarro, Navarro, Navarro, Navarro, Navarro, Navarro, Neistein, Nemmen, Neyman, Nulsen, Ocvirk, Okamoto, Okamoto, Omma, Oppenheimer, Ostriker, Owen, O’Shea, O’Shea, Padilla, Parkinson, Parrish, Parry, Peacock, Peacock, Peebles, Percival, Percival, Peters, Petkova, Pipino, Pipino, Plewa, Pontzen, Pope, Portinari, Prada, Press, Purcell, Putman, Quilis, Quinlan, Quinlan, Quinn, Randall, Rasmussen, Ratnatunga, Razoumov, Read, Read, Reed, Reed, Rees, Ricker, Ricotti, Ricotti, Ricotti, Rijkhorst, Robertson, Robertson, Robertson, Robertson, Robertson, Robinson, Romano, Romeo, Romeo, Roskar, Roskar, Roychowdhury, Rozo, Ruszkowski, Ruszkowski, Sales, Salpeter, Santoro, Scannapieco, Scannapieco, Scannapieco, Scannapieco, Schade, Schawinski, Schaye, Schmidt, Seljak, Sellwood, Sellwood, Sellwood, Sesana, Sesana, Shakura, Shapiro, Sharma, Shaw, Shen, Sheth, Shlosman, Sijacki, Silk, Silk, Silk, Silva, Simard, Slosar, Smith, Smith, Smoluchowksi, Somerville, Somerville, Somerville, Somerville, Somerville, Somerville, Spitzer, Spitzer, Springel, Springel, Springel, Springel, Springel, Springel, Stacy, Steinmetz, Stewart, Stinson, Strigari, Summers, Swinbank, Tasker, Tasker, Tassis, Taylor, Tegmark, Tegmark, Tegmark, Thacker, Thacker, Thorne, Tichy, Timmes, Tinker, Tinker, Tollerud, Toomre, Tormen, Toth, Tozzi, Tremaine, Tremaine, Trenti, Tumlinson, van den Bosch, van den Bosch, van den Bosch, van Dokkum, Vecchia, Vecchia, Veilleux, Velazquez, Vernaleo, Viel, Vikhlinin, Villalobos, Villiers, Vitvitska, Voit, Volonteri, Volonteri, Volonteri, Wadsley, Wang, Wang, Wang, Warren, Watanabe, Wechsler, Wechsler, Wen, White, White, White, White, White, Williams, Willman, Wise, Wise, Wise, Wise, Wise, Wise, Wuyts, Wyithe, Yajima, Yang, Yoshida, Yoshida, Yoshida, Younger, Younger, Yu, Yüksel, Zavala, Zhang, Zhao, Zhao, Zheng +563 morecore +4 more sourcesDLAs and Galaxy Formation [PDF]
Modern Physics Letters A, 2007 Damped Lyman-alpha systems (DLAs) are useful probes of star formation and
galaxy formation at high redshift. We study the physical properties of DLAs and
their relationship to Lyman-break galaxies using cosmological hydrodynamic
simulations based on the ...KENTARO NAGAMINE, Pettini M., York D. G.core +2 more sourcesGalaxy formation [PDF]
Proceedings of the National Academy of Sciences, 1998 It is argued that within the standard Big Bang cosmological model the bulk of the mass of the luminous parts of the large galaxies likely had been assembled by redshift z ∼ 10. Galaxy assembly this early would be difficult to fit in the widely discussed adiabatic cold dark matter model for structure formation ...Malcolm S. Longairsemanticscholar +5 more sourcesFormation of Galaxy Clusters [PDF]
Annual Review of Astronomy and Astrophysics, 2012 In this review, we describe our current understanding of cluster formation:
from the general picture of collapse from initial density fluctuations in an
expanding Universe to detailed simulations of cluster formation including the
effects of galaxy ...Andrey Kravtsov, Stefano Borganiexaly +3 more sourcesThe Formation of Galaxy Disks
, 2008 We present a new set of multi-million particle SPH simulations of the
formation of disk dominated galaxies in a cosmological context. Some of these
galaxies are higher resolution versions of the models already described in
Governato et al (2007).Brook, C., Governato, F., Mayer, L.core +3 more sourcesFractional yields inferred from halo and thick disk stars [PDF]
Serbian Astronomical Journal, 2013 Linear [Q/H]-[O/H] relations, Q = Na, Mg, Si, Ca, Ti, Cr, Fe, Ni, are
inferred from a sample (N = 67) of recently studied FGK-type dwarf stars in
the solar neighbourhood including different populations (Nissen and Schuster
2010, Ramirez et al ...Caimmi R.doaj +1 more sourceFormation of a Massive Lenticular Galaxy Under the Tidal Interaction with a Group of Dwarf Galaxies
The Astrophysical Journal Letters, 2023 Based on the atomic-hydrogen (H i ) observations using the Five-hundred-meter Aperture Spherical radio Telescope, we present a detailed study of the gas-rich massive S0 galaxy NGC 1023 in a nearby galaxy group.Jin-Long Xu, Ming Zhu, Kelley M. Hess, Naiping Yu, Chuan-Peng Zhang, Xiao-Lan Liu, Mei Ai, Peng Jiang, Jie Wang +8 moredoaj +1 more sourceThe epoch of galaxy formation [PDF]
Proceedings of the National Academy of Sciences, 1997 Recent advances in technology have enabled astronomers to observe fainter, and more distant, galaxies and to study the processes of galaxy formation and evolution. Recent observations suggest that the bulk of the stars in the universe formed between z = 3 (∼1 × 10^9 years after the big bang) and the present.Spergel, David N., Lilly, Simon J., Steidel, Charles C. +2 moreopenaire +3 more sources
