ISO spectroscopy of compact HII regions in our galaxy

被引：0

作者：

Martín-Hernández, NL ^{[1
]}

Peeters, E ^{[1
]}

Damour, F ^{[1
]}

Cox, P ^{[1
]}

Roelfsema, PR ^{[1
]}

Tielens, AGGM ^{[1
]}

Baluteau, JP ^{[1
]}

Churchwell, E ^{[1
]}

Jones, AP ^{[1
]}

Mathis, JS ^{[1
]}

Morisset, C ^{[1
]}

Schaerer, D ^{[1
]}

Kessler, MF ^{[1
]}

机构：

[1] Kapteyn Astron Inst, NL-9700 AV Groningen, Netherlands

来源：

ISO BEYOND THE PEAKS | 2000年 / 456卷

关键词：

Galaxy : abundances; HII regions; infrared : ISM : lines and bands : extinction; ISM : abundances;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report preliminary results of a study of the combined SWS-LWS grating spectra of compact H II regions in our Galaxy. The main goal of this study is to investigate the galactic abundance gradient. First results are presented together with a discussion of the problems and limitations of the present data set. In addition to the atomic finestructure lines, the spectra show a variety of dust features whose main characteristics are summarized.

引用

页码：135 / 140

页数：6

共 50 条

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