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Accurate oxygen abundance of interstellar gas in Mrk 71 from optical and infrared spectra - Nature Astronomy

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Accurate oxygen abundance of interstellar gas in Mrk 71 from optical and infrared spectra - Nature Astronomy

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 (Te) method are typically approximately two times lower than the values based on the recombination line method.

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Accurate oxygen abundance of interstellar gas in Mrk 71 from optical and infrared spectra - Nature Astronomy

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Accurate oxygen abundance of interstellar gas in Mrk 71 from optical and infrared spectra - Nature Astronomy

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