Comparing Galaxy Formation in Semi-Analytic Models and Hydrodynamical Simulations

Monthly Notices of the Royal Astronomical Society - United Kingdom
doi 10.1093/mnras/stx2770
Full Text
Abstract

Available in full text

Date
Authors
Publisher

Oxford University Press (OUP)

Related search

Cosmic Ray Feedback in Hydrodynamical Simulations of Galaxy Formation

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2007English

Cosmological Hydrodynamical Simulations of Galaxy Clusters: X-Ray Scaling Relations and Their Evolution

Monthly Notices of the Royal Astronomical Society
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Iron Abundances and Heating of the Intracluster Medium in Hydrodynamical Simulations of Galaxy Clusters

Monthly Notices of the Royal Astronomical Society
AstrophysicsAstronomyPlanetary ScienceSpace
2003English

Modelling the ISM and Star Formation in Galaxy Formation Simulations

Symposium - International Astronomical Union
2004English

Semi-Analytic Galaxy Evolution (Sage): Model Calibration and Basic Results

Astrophysical Journal, Supplement Series
AstrophysicsAstronomyPlanetary ScienceSpace
2016English

A New Semi-Analytic Model of Pop III Formation With Ultralarge Cosmological N-Body Simulations

2020English

The Eagle Simulations of Galaxy Formation: Public Release of Halo and Galaxy Catalogues

Astronomy and Computing
AstrophysicsComputer Science ApplicationsPlanetary ScienceAstronomySpace
2016English

Comparison of the Excess Mass Around CFHTLenS Galaxy-Pairs to Predictions From a Semi-Analytic Model Using Galaxy-Galaxy-Galaxy Lensing

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Bubbles in Collision: Hydrodynamical Models

International Astronomical Union Colloquium
1997English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy