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Direct measures of chemical abundances from stacked spectra of star-forming galaxies: Implications f...

Direct measures of chemical abundances from stacked spectra of star-forming galaxies: Implications f...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2506160218

Direct measures of chemical abundances from stacked spectra of star-forming galaxies: Implications for the mass–metallicity–star formation rate relation

About this item

Full title

Direct measures of chemical abundances from stacked spectra of star-forming galaxies: Implications for the mass–metallicity–star formation rate relation

Publisher

Cambridge, UK: Cambridge University Press

Journal title

Proceedings of the International Astronomical Union, 2020-03, Vol.15 (S359), p.424-426

Language

English

Formats

Publication information

Publisher

Cambridge, UK: Cambridge University Press

More information

Scope and Contents

Contents

The stellar mass–star formation rate–metallicity relation provides clues on the chemical evolution of galaxies. We revisit this relation by measuring the gas-phase metallicity using the direct method. For metal-rich galaxies this is not straightforward, because auroral emission lines sensitive the electron temperature are lost in spectral noise. In...

Alternative Titles

Full title

Direct measures of chemical abundances from stacked spectra of star-forming galaxies: Implications for the mass–metallicity–star formation rate relation

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2506160218

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2506160218

Other Identifiers

ISSN

1743-9213

E-ISSN

1743-9221

DOI

10.1017/S174392132000188X

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