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 shape of dark matter haloes - II. The GALACTUS HI modelling & fitting tool

dc.contributor.authorPeters, S. P C
dc.contributor.authorvan der Kruit, P C
dc.contributor.authorAllen, R J
dc.contributor.authorFreeman, Kenneth
dc.date.accessioned2020-12-20T20:58:13Z
dc.date.available2020-12-20T20:58:13Z
dc.date.issued2017
dc.date.updated2020-11-23T11:20:34Z
dc.description.abstractWe present a new HI modelling tool called GALACTUS. The program has been designed to perform automated fits of disc-galaxy models to observations. It includes a treatment for the self-absorption of gas. The software has been released into the public domain.We describe the design philosophy and inner workings of the program. After this, we model the face-on galaxy NGC 2403 using both self-absorption and optically thin models, showing that self-absorption occurs even in face-on galaxies. These results are then used to model an edge-on galaxy. It is shown that the maximum surface brightness plateaus seen in Paper I of this series are indeed signs of self-absorption. The apparent HI mass of an edge-on galaxy can be drastically lower compared with that same galaxy seen face-on. The Tully-Fisher relation is found to be relatively free from self-absorption issues
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/218524
dc.language.isoen_AUen_AU
dc.publisherBlackwell Publishing Ltd
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.titleThe shape of dark matter haloes - II. The GALACTUS HI modelling & fitting tool
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage31
local.bibliographicCitation.startpage21
local.contributor.affiliationPeters, S. P C, University of Groningen, Kapteyn Astronomical Institute
local.contributor.affiliationvan der Kruit, P C, University of Groningen Kapteyn Astronomical Institute
local.contributor.affiliationAllen, R J, Space Telescope Science Institute
local.contributor.affiliationFreeman, Kenneth, College of Science, ANU
local.contributor.authoruidFreeman, Kenneth, u7000399
local.description.notesImported from ARIES
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.ariespublicationa383154xPUB5372
local.identifier.citationvolume464
local.identifier.doi10.1093/mnras/stw2099
local.identifier.scopusID2-s2.0-85014791690
local.identifier.thomsonID000393646300002
local.type.statusPublished Version

Downloads

abcd