4.7 Article

On the relation between electron temperatures in the O+ and O++ zones in high-metallicity HII regions

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OXFORD UNIV PRESS
DOI: 10.1111/j.1365-2966.2006.10618.x

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ISM : abundances; HII regions; galaxies : abundances

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We suggest a new way to establish the relation between the electron temperature t(3) within the [O III] zone and the electron temperature t(2) within the [O II] zone in high-metallicity (12 + log(O/H) > 8.25) H II regions. The t(2)-t(3) diagram is constructed by applying our method to a sample of 372 H II regions. We find that the correlation between t2 and t3 is tight and can be approximated by a linear expression. The new t(2)-t(3) relation can be used to determine t2 and accurate abundances in high-metallicity H II regions with a measured t3. It can also be used in conjunction with the ff relation for the determination of t3 and t2 and oxygen abundances in high-metallicity H II regions, where the [O III]lambda 4363 auroral line is not detected. The derived t(2)-t(3) relation is independent of photoionization models of H II regions.

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