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

被引:33
|
作者
Pilyugin, Leonid S.
Vilchez, Jose M.
Thuan, Trinh X.
机构
[1] Natl Acad Sci Ukraine, Main Astron Observ, UA-03680 Kiev, Ukraine
[2] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain
[3] Univ Virginia, Dept Astron, Charlottesville, VA 22903 USA
关键词
ISM : abundances; HII regions; galaxies : abundances;
D O I
10.1111/j.1365-2966.2006.10618.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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.
引用
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页码:1928 / 1934
页数:7
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