Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/30800
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Wang, Jing | en_US |
dc.contributor.author | Koribalski, Bärbel S. | en_US |
dc.contributor.author | SERRA, PAOLO | en_US |
dc.contributor.author | van der Hulst, Thijs | en_US |
dc.contributor.author | Roychowdhury, Sambit | en_US |
dc.contributor.author | Kamphuis, Peter | en_US |
dc.contributor.author | Chengalur, Jayaram N. | en_US |
dc.date.accessioned | 2021-04-19T15:36:58Z | - |
dc.date.available | 2021-04-19T15:36:58Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/30800 | - |
dc.description.abstract | We revisit the H I size-mass (D_{H I}-M<SUB>H I</SUB>) relation of galaxies with a sample of more than 500 nearby galaxies covering over five orders of magnitude in H I mass and more than 10 B-band magnitudes. The relation is remarkably tight with a scatter σ ∼ 0.06 dex, or 14 per cent. The scatter does not change as a function of galaxy luminosity, H I richness or morphological type. The relation is linked to the fact that dwarf and spiral galaxies have a homogeneous radial profile of H I surface density in the outer regions when the radius is normalized by D<SUB>H I</SUB>. The early-type disc galaxies typically have shallower H I radial profiles, indicating a different gas accretion history. We argue that the process of atomic-to-molecular gas conversion or star formation cannot explain the tightness of the D<SUB>H I</SUB>-M<SUB>H I</SUB> relation. This simple relation puts strong constraints on simulation models for galaxy formation. | en_US |
dc.language.iso | eng | en_US |
dc.title | New lessons from the H I size-mass relation of galaxies | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stw1099 | en_US |
dc.identifier.scopus | 2-s2.0-84983043990 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/460/2/2143/2609089 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 460 | en_US |
dc.relation.issue | 2 | en_US |
dc.relation.firstpage | 2143 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2016MNRAS.460.2143W | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
item.languageiso639-1 | en | - |
item.openairetype | Article | - |
item.cerifentitytype | Publications | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
crisitem.author.dept | O.A. Cagliari | - |
crisitem.author.orcid | 0000-0001-5965-252X | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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stw1099.pdf | Pdf editoriale | 1.63 MB | Adobe PDF | View/Open |
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