The Auriga Project: the properties and formation mechanisms of disc galaxies across cosmic time
暂无分享,去创建一个
Federico Marinacci | Carlos S. Frenk | Volker Springel | Simon D. M. White | Ruediger Pakmor | S. White | V. Springel | C. Frenk | A. Jenkins | F. G'omez | R. Grand | F. Marinacci | R. Pakmor | Adrian Jenkins | Facundo A. G'omez | Robert J. J. Grand | David J. R. Campbell | D. Campbell | S. White
[1] M. Zaldarriaga,et al. Submitted to ApJ Preprint typeset using L ATEX style emulateapj v. 10/09/06 A NEW CALCULATION OF THE IONIZING BACKGROUND SPECTRUM AND THE EFFECTS OF HEII REIONIZATION , 2022 .
[2] S. White,et al. The EAGLE project: Simulating the evolution and assembly of galaxies and their environments , 2014, 1407.7040.
[3] S. White,et al. The formation and survival of discs in a ΛcDM universe , 2008, 0812.0976.
[4] Phillip James Edwin Peebles,et al. Origin of the Angular Momentum of Galaxies , 1969 .
[5] P. Hopkins,et al. The structure of the interstellar medium of star‐forming galaxies , 2011, 1110.4636.
[6] J. Wadsley,et al. A Superbubble Feedback Model for Galaxy Simulations , 2014, 1405.2625.
[7] V. Springel,et al. Feedback and the structure of simulated galaxies at redshift z=2 , 2010, 1004.5386.
[8] Durham,et al. What Shapes the Luminosity Function of Galaxies? , 2003, astro-ph/0302450.
[9] J. Newman,et al. On the evolution of the velocity–mass–size relations of disc-dominated galaxies over the past 10 billion years , 2010, 1006.3558.
[10] A. Karakas. Updated stellar yields from asymptotic giant branch models , 2009, 0912.2142.
[11] Junichiro Makino,et al. A DENSITY-INDEPENDENT FORMULATION OF SMOOTHED PARTICLE HYDRODYNAMICS , 2012, 1202.4277.
[12] J. Schombert,et al. WEIGHING GALAXY DISKS WITH THE BARYONIC TULLY–FISHER RELATION , 2015, 1501.06826.
[13] R. Teyssier,et al. The formation of disc galaxies in a ΛCDM universe , 2010, 1004.0005.
[14] S. M. Fall,et al. Formation and rotation of disc galaxies with haloes , 1980 .
[15] V. Springel,et al. Simulating galaxy formation with black hole driven thermal and kinetic feedback , 2016, 1607.03486.
[16] G. Magdis,et al. On the stellar masses of IRAC detected Lyman Break Galaxies at z∼ 3 , 2009, 0909.3950.
[17] M. Steinmetz,et al. Simulations of Galaxy Formation in a Λ Cold Dark Matter Universe. I. Dynamical and Photometric Properties of a Simulated Disk Galaxy , 2002, astro-ph/0211331.
[18] A. Jenkins,et al. Second-order Lagrangian perturbation theory initial conditions for resimulations , 2009, 0910.0258.
[19] J. Bailin,et al. Cosmological galaxy formation simulations using smoothed particle hydrodynamics , 2010 .
[20] R. Nichol,et al. Stellar masses and star formation histories for 105 galaxies from the Sloan Digital Sky Survey , 2002, astro-ph/0204055.
[21] V. Springel,et al. A unified model for AGN feedback in cosmological simulations of structure formation , 2007, 0705.2238.
[22] Zurich,et al. MaGICC thick disc - I. Comparing a simulated disc formed with stellar feedback to the Milky Way , 2013, 1301.5318.
[23] T. Thompson,et al. Numerical simulations of radiatively driven dusty winds , 2013, 1302.4440.
[24] V. Springel,et al. Introducing the Illustris Project: the evolution of galaxy populations across cosmic time , 2014, 1405.3749.
[25] Daisuke Kawata,et al. GCD+: a new chemodynamical approach to modelling supernovae and chemical enrichment in elliptical galaxies , 2003 .
[26] David Schlegel,et al. The Milky Way Tomography with SDSS. I. Stellar Number Density Distribution , 2005, astro-ph/0510520.
[27] C. Flynn,et al. On the mass-to-light ratio of the local Galactic disc and the optical luminosity of the Galaxy , 2006, astro-ph/0608193.
[28] G. Stinson,et al. Star formation and feedback in smoothed particle hydrodynamic simulations – I. Isolated galaxies , 2006, astro-ph/0602350.
[29] U. Durham,et al. How supernova explosions power galactic winds , 2012, 1211.1395.
[30] O. Valenzuela,et al. COSMOLOGICAL SIMULATIONS OF MILKY WAY-SIZED GALAXIES , 2016, 1607.07917.
[31] Neal Katz,et al. Dissipational galaxy formation. II - Effects of star formation , 1992 .
[32] P. Roe,et al. A Solution-Adaptive Upwind Scheme for Ideal Magnetohydrodynamics , 1999 .
[33] B. Gibson,et al. Hierarchical formation of bulgeless galaxies: why outflows have low angular momentum , 2010, 1010.1004.
[34] V. Springel,et al. Cosmological smoothed particle hydrodynamics simulations: a hybrid multiphase model for star formation , 2002, astro-ph/0206393.
[35] Mattia Fumagalli,et al. THE STRUCTURAL EVOLUTION OF MILKY-WAY-LIKE STAR-FORMING GALAXIES SINCE z ∼ 1.3 , 2013, 1304.2395.
[36] F. Hoyle,et al. On the Mechanism of Accretion by Stars , 1944 .
[37] A. Cimatti,et al. Multiwavelength Study of Massive Galaxies at z~2. I. Star Formation and Galaxy Growth , 2007, 0705.2831.
[38] B. Oppenheimer,et al. Cosmological simulations of intergalactic medium enrichment from galactic outflows , 2006, astro-ph/0605651.
[39] V. Springel,et al. Zooming in on major mergers: dense, starbursting gas in cosmological simulations , 2016, 1604.08205.
[40] V. Springel,et al. Shaping the galaxy stellar mass function with supernova- and AGN-driven winds , 2012, 1205.2694.
[41] D. Kawata. Effects of Type II and Type Ia Supernovae Feedback on the Chemodynamical Evolution of Elliptical Galaxies , 2001, astro-ph/0105297.
[42] P. Hopkins,et al. Forward and backward galaxy evolution in comoving cumulative number density space , 2016, 1606.07271.
[43] J. Schaye,et al. The Aquila comparison project: the effects of feedback and numerical methods on simulations of galaxy formation , 2011, 1112.0315.
[44] C. Dobbs,et al. Testing hydrodynamics schemes in galaxy disc simulations , 2016, 1605.09792.
[45] M. Steinmetz,et al. ON THE ORIGIN OF THE ANGULAR MOMENTUM PROPERTIES OF GAS AND DARK MATTER IN GALACTIC HALOS AND ITS IMPLICATIONS , 2012, 1203.0315.
[46] J. Gunn,et al. Dissipational Galaxy Formation. I. Effects of Gasdynamics , 1991 .
[47] J. Schaye,et al. Simulating galactic outflows with kinetic supernova feedback , 2008, 0801.2770.
[48] J. Schaye,et al. Simulating galactic outflows with thermal supernova feedback , 2012, 1203.5667.
[49] E. Ostriker,et al. GALAXY OUTFLOWS WITHOUT SUPERNOVAE , 2016, 1601.00659.
[50] V. Springel,et al. The formation of disc galaxies in high-resolution moving-mesh cosmological simulations , 2013, 1305.5360.
[51] A. Dekel,et al. A Universal Angular Momentum Profile for Galactic Halos , 2000, astro-ph/0011001.
[52] G. Stinson,et al. NIHAO VI. The hidden discs of simulated galaxies , 2016, 1603.01703.
[53] S. Courteau,et al. Scaling Relations of Spiral Galaxies , 2007, 0708.0422.
[54] Angular momentum transport and disc morphology in smoothed particle hydrodynamics simulations of galaxy formation , 2006, astro-ph/0601115.
[55] Lucio Mayer,et al. FORMING REALISTIC LATE-TYPE SPIRALS IN A ΛCDM UNIVERSE: THE ERIS SIMULATION , 2011, 1103.6030.
[56] O. Agertz,et al. Resolving mixing in smoothed particle hydrodynamics , 2009, 0906.0774.
[57] T. Okamoto. The origin of pseudo-bulges in cosmological simulations of galaxy formation , 2012, 1203.5372.
[58] Effects of feedback on the morphology of galaxy discs , 2005, astro-ph/0503676.
[59] Matthew A. Bershady,et al. THE DISKMASS SURVEY. I. OVERVIEW , 2010, 1004.4816.
[60] S. White,et al. Warps and waves in the stellar discs of the Auriga cosmological simulations , 2016, 1606.06295.
[61] Liverpool John Moores University,et al. Bent by baryons: the low-mass galaxy-halo relation , 2014, 1404.3724.
[62] H. Bondi,et al. On spherically symmetrical accretion , 1952 .
[63] Piet Hut,et al. A hierarchical O(N log N) force-calculation algorithm , 1986, Nature.
[64] T. Naab,et al. The energy and momentum input of supernova explosions in structured and ionized molecular clouds , 2014, 1410.0011.
[65] D. Gadotti. Structural properties of pseudo-bulges, classical bulges and elliptical galaxies: a Sloan Digital Sky Survey perspective , 2008, 0810.1953.
[66] G. Bruzual,et al. Stellar population synthesis at the resolution of 2003 , 2003, astro-ph/0309134.
[67] C. Simpson,et al. Simulating cosmic ray physics on a moving mesh , 2016, 1604.07399.
[68] R. Bower,et al. The EAGLE simulations of galaxy formation: the importance of the hydrodynamics scheme , 2015, 1509.05056.
[69] J. Silk,et al. AGN-driven quenching of star formation: morphological and dynamical implications for early-type galaxies , 2013, 1301.3092.
[70] P. Hopkins,et al. (Star)bursts of FIRE: observational signatures of bursty star formation in galaxies , 2015, 1510.03869.
[71] Michael Kuhlen,et al. Dark Matter Substructure and Gamma-Ray Annihilation in the Milky Way Halo , 2006, astro-ph/0611370.
[72] S. White,et al. Effects of supernova feedback on the formation of galaxy discs , 2008, 0804.3795.
[73] Cfa,et al. The large-scale properties of simulated cosmological magnetic fields , 2015, 1506.00005.
[74] V. Springel,et al. Simulations of magnetic fields in isolated disc galaxies , 2012, 1212.1452.
[75] Timothy D. Brandt,et al. The delay-time distribution of Type Ia supernovae from Sloan II , 2012, 1206.0465.
[76] G. Stinson,et al. NIHAO project – I. Reproducing the inefficiency of galaxy formation across cosmic time with a large sample of cosmological hydrodynamical simulations , 2015, 1503.04818.
[77] Making Galaxies in a Cosmological Context: The Need for Early Stellar Feedback , 2012, 1208.0002.
[78] V. Springel. E pur si muove: Galilean-invariant cosmological hydrodynamical simulations on a moving mesh , 2009, 0901.4107.
[79] P. Hopkins,et al. Galaxies on FIRE (Feedback In Realistic Environments): stellar feedback explains cosmologically inefficient star formation , 2013, 1311.2073.
[80] V. Springel,et al. A model for cosmological simulations of galaxy formation physics: multi-epoch validation , 2013, 1305.4931.
[81] V. Springel. The Cosmological simulation code GADGET-2 , 2005, astro-ph/0505010.
[82] T. D. Matteo,et al. Modelling feedback from stars and black holes in galaxy mergers , 2004, astro-ph/0411108.
[83] H. Rix,et al. THE STAR FORMATION HISTORY OF MASS-SELECTED GALAXIES IN THE COSMOS FIELD , 2010, 1011.6370.
[84] R. Teyssier,et al. Baryonic and dark matter distribution in cosmological simulations of spiral galaxies , 2014, Monthly Notices of the Royal Astronomical Society.
[85] B. Willman,et al. Bulgeless dwarf galaxies and dark matter cores from supernova-driven outflows , 2009, Nature.
[86] S. White,et al. Properties of H i discs in the Auriga cosmological simulations , 2016, 1610.01594.
[87] Bingqiu Chen,et al. The Milky Way's rotation curve out to 100 kpc and its constraint on the Galactic mass distribution , 2016, 1604.01216.
[88] R. Teyssier,et al. A systematic look at the effects of radiative feedback on disc galaxy formation , 2013, 1308.6321.
[89] A. Hopkins,et al. Galaxy And Mass Assembly (GAMA): $\mathcal {M_\star }-R_{\rm e}$ relations of z = 0 bulges, discs and spheroids , 2016, 1607.01096.
[90] C. Brook,et al. INTERPRETING THE EVOLUTION OF THE SIZE–LUMINOSITY RELATION FOR DISK GALAXIES FROM REDSHIFT 1 TO THE PRESENT , 2010, 1011.0432.
[91] S. White,et al. The inner structure of ΛCDM haloes – I. A numerical convergence study , 2002, astro-ph/0201544.
[92] V. Springel,et al. Vertical disc heating in Milky Way-sized galaxies in a cosmological context , 2015, 1512.02219.
[93] Federico Marinacci,et al. Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation , 2014, 1403.4934.
[94] Shude Mao,et al. The formation of galactic discs , 1997 .
[95] G. Efstathiou,et al. The evolution of large-scale structure in a universe dominated by cold dark matter , 1985 .
[96] Durham,et al. The properties of satellite galaxies in simulations of galaxy formation , 2009, 0909.0265.
[97] V. Springel,et al. Angular momentum properties of haloes and their baryon content in the Illustris simulation , 2016, 1608.01323.
[98] Iap,et al. The ages and metallicities of galaxies in the local universe , 2005, astro-ph/0506539.
[99] Durham,et al. The Aquarius Project: the subhaloes of galactic haloes , 2008, 0809.0898.
[100] S. White,et al. A fully cosmological model of a Monoceros-like ring , 2015, 1509.08459.
[101] A. Fabian,et al. Fuelling quasars with hot gas , 1999, astro-ph/9908282.
[102] M. Steinmetz,et al. Dark Halo and Disk Galaxy Scaling Laws in Hierarchical Universes , 2000, astro-ph/0001003.
[103] Andreas Bauer,et al. Shocking results without shocks: Subsonic turbulence in smoothed particle hydrodynamics and moving-mesh simulations , 2011, 1109.4413.
[104] Durham,et al. Baryon effects on the internal structure of ΛCDM haloes in the EAGLE simulations , 2014, 1409.8617.
[105] Thorsten Naab,et al. Towards a more realistic population of bright spiral galaxies in cosmological simulations , 2013, 1304.1559.
[106] S. White,et al. Galactic star formation and accretion histories from matching galaxies to dark matter haloes , 2012, 1205.5807.
[107] A. Kravtsov,et al. FUEL EFFICIENT GALAXIES: SUSTAINING STAR FORMATION WITH STELLAR MASS LOSS , 2010, 1011.1252.
[108] S. White,et al. Simulations of dissipative galaxy formation in hierarchically clustering universes – II. Dynamics of the baryonic component in galactic haloes , 1994 .
[109] R. Wechsler,et al. The Origin of Angular Momentum in Dark Matter Halos , 2001, astro-ph/0105349.
[110] D. Wake,et al. 3D-HST+CANDELS: THE EVOLUTION OF THE GALAXY SIZE–MASS DISTRIBUTION SINCE z = 3 , 2014, 1404.2844.
[111] A. Jenkins. A new way of setting the phases for cosmological multiscale Gaussian initial conditions. , 2013, 1306.5968.
[112] Volker Springel,et al. Improving the convergence properties of the moving-mesh code AREPO , 2015, 1503.00562.
[113] S. White,et al. How do galaxies populate dark matter haloes , 2009, 0909.4305.
[114] A. Mezzacappa,et al. Nuclear cross sections, nuclear structure and stellar nucleosynthesis , 2003 .