Panchromatic star formation rate indicators and their uncertainties
Panchromatic star formation rate indicators and their uncertainties
About this item
Full title
Author / Creator
Publisher
Cambridge, UK: Cambridge University Press
Journal title
Language
English
Formats
Publication information
Publisher
Cambridge, UK: Cambridge University Press
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More information
Scope and Contents
Contents
The star formation rate (SFR) is a fundamental property of galaxies and it is crucial to understand the build-up of their stellar content, their chemical evolution, and energetic feedback. The SFR of galaxies is typically obtained by observing the emission by young stellar populations directly in the ultraviolet, the optical nebular line emission f...
Alternative Titles
Full title
Panchromatic star formation rate indicators and their uncertainties
Authors, Artists and Contributors
Author / Creator
Identifiers
Primary Identifiers
Record Identifier
TN_cdi_proquest_miscellaneous_1880031534
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_1880031534
Other Identifiers
ISSN
1743-9213
E-ISSN
1743-9221
DOI
10.1017/S1743921316004816
