Relevant bibliographies by topics / Semi-analytic models

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  1. Journal articles

Academic literature on the topic 'Semi-analytic models'

Author: Grafiati
Published: 1 April 2023

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Journal articles on the topic "Semi-analytic models"

1

Lacerna, I., S. Contreras, R. E. González, N. Padilla, and V. Gonzalez-Perez. "Galactic conformity measured in semi-analytic models." Monthly Notices of the Royal Astronomical Society 475, no. 1 (2017): 1177–89. http://dx.doi.org/10.1093/mnras/stx3253.

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2

Hartl, Urs T. "Semi-stable models for rigid-analytic spaces." manuscripta mathematica 110, no. 3 (2003): 365–80. http://dx.doi.org/10.1007/s00229-002-0349-x.

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3

Gruppioni, C., F. Calura, F. Pozzi, et al. "Star formation inHerschel's Monsters versus semi-analytic models." Monthly Notices of the Royal Astronomical Society 451, no. 4 (2015): 3419–26. http://dx.doi.org/10.1093/mnras/stv1204.

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4

Visbal, Eli, Zoltán Haiman, and Greg L. Bryan. "Self-consistent semi-analytic models of the first stars." Monthly Notices of the Royal Astronomical Society 475, no. 4 (2018): 5246–56. http://dx.doi.org/10.1093/mnras/sty142.

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5

Donnelly, IJ, EK Rose, and JL Cook. "Magnetohydrodynamic Equilibrium Models for Rotamak Plasmas." Australian Journal of Physics 40, no. 2 (1987): 175. http://dx.doi.org/10.1071/ph870175.

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A semi-analytic method is used to solve the Grad-Shafranov equation for a range of compact torus plasma configurations which have ellipsoidal separatrices, zero toroidal magnetic field and pressure P proportional to the square of the poloidal flux function 1[1. The equilibria are compared with the analytic solutions of the Solov'ev model, for which P ex 1[1.
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6

Delfino, Facundo M., Claudia G. Scóccola, Sofía A. Cora, Cristian A. Vega-Martínez, and Ignacio D. Gargiulo. "Tracking the orbit of unresolved subhaloes for semi-analytic models." Monthly Notices of the Royal Astronomical Society 510, no. 2 (2021): 2900–2919. http://dx.doi.org/10.1093/mnras/stab3494.

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ABSTRACT We present a model to track the orbital evolution of ‘unresolved subhaloes’ (USHs) in cosmological simulations. USHs are subhaloes that are no longer distinguished by halo finders as self-bound overdensities within their larger host system due to limited mass resolution. These subhaloes would host ‘orphan galaxies’ in semi-analytic models of galaxy formation and evolution (SAMs). Predicting the evolution of the phase-space components of USHs is crucial for the adequate modelling of environmental processes, interactions, and mergers implemented in SAMs that affect the baryonic properti
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7

Mitchell, Peter D., Cedric G. Lacey, Claudia D. P. Lagos, et al. "Comparing galaxy formation in semi-analytic models and hydrodynamical simulations." Monthly Notices of the Royal Astronomical Society 474, no. 1 (2017): 492–521. http://dx.doi.org/10.1093/mnras/stx2770.

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8

Yates, Robert M., Bruno Henriques, Peter A. Thomas, Guinevere Kauffmann, Jonas Johansson, and Simon D. M. White. "Modelling element abundances in semi-analytic models of galaxy formation." Monthly Notices of the Royal Astronomical Society 435, no. 4 (2013): 3500–3520. http://dx.doi.org/10.1093/mnras/stt1542.

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9

Henriques, Bruno M., Serena Bertone, and Peter A. Thomas. "The effect of dwarf galaxy disruption in semi-analytic models." Monthly Notices of the Royal Astronomical Society 383, no. 4 (2007): 1649–54. http://dx.doi.org/10.1111/j.1365-2966.2007.12684.x.

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10

Brennan, Ryan, Viraj Pandya, Rachel S. Somerville, et al. "Quenching and morphological transformation in semi-analytic models and CANDELS." Monthly Notices of the Royal Astronomical Society 451, no. 3 (2015): 2933–56. http://dx.doi.org/10.1093/mnras/stv1007.

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