The electron-impact broadening effect in hot star atmospheres: The case of singly- and doubly-ionized zirconium

被引：27

作者：

Popovic, LC ^{[1
]}

Milovanovic, N ^{[1
]}

Dimitrijevic, MS ^{[1
]}

机构：

[1] Astron Observ, YU-11160 Serbia 74, Yugoslavia

来源：

ASTRONOMY & ASTROPHYSICS | 2001年 / 365卷 / 03期

关键词：

atomic data; plasma; stars : atmospheres;

D O I：

10.1051/0004-6361:20000013

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The electron-impact widths for 30 Zr III lines were calculated using the modified semi-empirical (MSE) method. For two Zr IE and four Zr III astrophysically important UV lines, only electron-impact widths are given, since for their calculation the experimental oscillator strengths were used and consequently the accuracy of the parameters is lower than in the case of other lines. The influence of the electron-impact mechanism on line shapes and equivalent widths in hot star atmospheres was also considered. The impact of the electron-impact broadening effect on abundance determination, particularly its effect on "zirconium conflict" is discussed as well.

引用

页码：656 / 659

页数：4

共 31 条

[1] THE CALCULATION OF THE ABSOLUTE STRENGTHS OF SPECTRAL LINES [J].