Test environment running 7.6.6

Cultural advice

The Australian National University acknowledges, celebrates and pays our respects to the Ngunnawal and Ngambri people of the Canberra region and to all First Nations Australians on whose traditional lands we meet and work, and whose cultures are among the oldest continuing cultures in human history.

Aboriginal and Torres Strait Islander peoples are advised that ANU Library collections may include images, names, voices, and other representations of deceased persons.

Material in the collection may contain terms, language or views that reflect the period in which the item was created and may be considered inappropriate today.

The Aquila comparison project: The effects of feedback and numerical methods on simulations of galaxy formation

Thumbnail Image

Date

2012

Authors

Scannapieco, C
Wadepuhl, M
Parry, O H
Navarro, J F
Jenkins, Adrian
Springel, V
Teyssier, R
Carlson, E
Couchman, H M P
Crain, R A

Journal Title

Journal ISSN

Volume Title

Publisher

Blackwell Publishing Ltd

Abstract

We compare the results of various cosmological gas-dynamical codes used to simulate the formation of a galaxy in the Λ cold dark matter structure formation paradigm. The various runs (13 in total) differ in their numerical hydrodynamical treatment [smoot

Description

Keywords

Citation

URI

http://hdl.handle.net/1885/66355

Collections

Open Access Research

Source

Monthly Notices of the Royal Astronomical Society

Type

Journal article

Book Title

Entity type

Access Statement

License Rights

DOI

10.1111/j.1365-2966.2012.20993.x

Restricted until

2037-12-31

Downloads

File
Description
01_Scannapieco_The_Aquila_comparison_project:_2012.pdf (2.77 MB)

DSpace software copyright © 2002-2026 LYRASIS