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Star Formation during Galaxy Formation [PDF]
EAS Publications Series, 2011 Young galaxies are clumpy, gas-rich, and highly turbulent. Star formation
appears to occur by gravitational instabilities in galactic disks. The high
dispersion makes the clumps massive and the disks thick. The star formation
rate should be comparable to the gas accretion rate of the whole galaxy,
because star formation is usually rapid and the gas ...Abraham, Agertz, B.G. Elmegreen, Barden, Bigiel, Birnboim, Blitz, Bouche, Bournaud, Bournaud, Bournaud, Brooks, Burkert, Casini, Casini, Ceverino, Choi, Conselice, Cowie, Daddi, Daddi, Daddi, Daddi, Dekel, Dekel, Dekel, Ebisuzaki, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Elmegreen, Förster, Förster-Schreiber, Garland, Genzel, Genzel, Genzel, Heckman, Immeli, Immeli, Kennicutt, Kereŝ, Kereŝ, Law, Maehara, McKee, Murali, Noeske, Noguchi, Ocvirk, Overzier, Overzier, Overzier, Petty, Portegies-Zwart, Puech, Quinn, Schaye, Semelin, Shapiro, Springel, Tacconi, van den Bergh, Walker, Weiner, Yoachim +75 morearxiv +7 more sourcesGalaxy 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 +6 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 V. Kravtsov, Audit E, Binney J, Bower RG, Brunetti G, Courtin J, Doroshkevich AG, Einasto J, Ettori S, Gott JR, Hubble EP, Klypin AA, Mantz A, Mantz A, McCarthy IG, O'Shea BW, Stefano Borgani, Sunyaev RA, Sunyaev RA, Sunyaev RA, Tissera PB, van Albada GB, Wagner C, Zel'dovich YB, Zwicky F +24 morecore +6 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 +4 more sourcesFeedback in Galaxy Formation [PDF]
Proceedings of the International Astronomical Union, 2011 I review the outstanding problems in galaxy formation theory, and the role of
feedback in resolving them. I address the efficiency of star formation, the
galactic star formation rate, and the roles of supernovae and supermassive
black holes.Comment: To ...Antonuccio-Delogu, Boomsma, Heald, Joseph Silk, LeAAAABorne, Norman +5 morecore +6 more sourcesQuasars and galaxy formation [PDF]
Monthly Notices of the Royal Astronomical Society, 1999 Quasars are widely believed to be powered by accretion onto supermassive
black holes and there is now considerable evidence for a link between mergers,
quasars and the formation of spheroids. Cattaneo, Haehnelt & Rees (1999) have
demonstrated that a very A. Cattaneo, Copi, Schrammcore +6 more sourcesHow do galaxies get their baryons? [PDF]
, 2011 Understanding how galaxies obtain baryons, their stars and gas, over cosmic
time is traditionally approached in two different ways - theoretically and
observationally. In general, observational approaches to galaxy formation
include measuring basic galaxy properties, such as luminosities, stellar
masses, rotation speeds, star formation rates and how ...Conselice, Christopher J.arxiv +3 more sourcesQuantitative Estimates of Environmental Effects on the Star Formation
Rate of Disk Galaxies in Clusters of Galaxies [PDF]
, 1998 A simple model is constructed to evaluate the change of star formation rate
of a disk galaxy due to environmental effects in clusters of galaxies. Three
effects, (1) tidal force from the potential well of the cluster, (2) increase
of external pressure when the galaxy plows into the intracluster medium, (3)
high-speed encounters between galaxies, are ...Evrard A. E., Fritze, Gusten R, Maeder A., Mihara K., Navarro J. F., Yutaka Fujita +6 morearxiv +4 more sourcesCosmological Constraints from Galaxy Clustering and the Mass-to-Number
Ratio of Galaxy Clusters: Marginalizing over the Physics of Galaxy Formation [PDF]
, 2013 Many approaches to obtaining cosmological constraints rely on the connection
between galaxies and dark matter. However, the distribution of galaxies is
dependent on their formation and evolution as well as the cosmological model,
and galaxy formation is still not a well-constrained process.Lu, Yu, Reddick, Rachel, Tinker, Jeremy, Wechsler, Risa +3 morearxiv +4 more sources
