Gas accretion as the origin of chemical abundance gradients in distant galaxies
Gas accretion as the origin of chemical abundance gradients in distant galaxies
About this item
Full title
Author / Creator
Cresci, G. , Mannucci, F. , Maiolino, R. , Marconi, A. , Gnerucci, A. and Magrini, L.
Publisher
London: Nature Publishing Group UK
Journal title
Language
English
Formats
Publication information
Publisher
London: Nature Publishing Group UK
Subjects
More information
Scope and Contents
Contents
Cool gas fuels star formation
Although it is thought that some galaxies in the early Universe grew rapidly through violent mergers, the properties of many early galaxies are incompatible with that scenario. Cresci
et al
. now report chemical abundance data from three star-forming galaxies at redshift
z
= 3 — equivalent to only two bi...
Alternative Titles
Full title
Gas accretion as the origin of chemical abundance gradients in distant galaxies
Authors, Artists and Contributors
Author / Creator
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_miscellaneous_758835285
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_758835285
Other Identifiers
ISSN
0028-0836
E-ISSN
1476-4687
DOI
10.1038/nature09451
