Accurate oxygen abundance of interstellar gas in Mrk 71 from optical and infrared spectra
Accurate oxygen abundance of interstellar gas in Mrk 71 from optical and infrared spectra
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London: Nature Publishing Group UK
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Language
English
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London: Nature Publishing Group UK
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Contents
The heavy element content (‘metallicity’) of the Universe is a record of the total star formation history. Gas-phase metallicity in galaxies, as well as its evolution with time, is of particular interest as a tracer of accretion and outflow processes. However, metallicities from the widely used electron temperature (
T
e
) method are typic...
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Full title
Accurate oxygen abundance of interstellar gas in Mrk 71 from optical and infrared spectra
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TN_cdi_proquest_journals_2839656305
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2839656305
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ISSN
2397-3366
E-ISSN
2397-3366
DOI
10.1038/s41550-023-01953-7
