Oxygen and helium abundances in Galactic HII regions -: I.: Observations

被引:45
作者
Caplan, J
Deharveng, L
Peña, M
Costero, R
Blondel, C
机构
[1] Observ Marseille, F-13248 Marseille 4, France
[2] Univ Nacl Autonoma Mexico, Inst Astron, Mexico City 04510, DF, Mexico
[3] CEA Saclay, DAPNIA, Serv Astrophys, F-91191 Gif Sur Yvette, France
关键词
instrumentation : miscellaneous; techniques : photometric; ISM : abundances; HII regions;
D O I
10.1046/j.1365-8711.2000.03029.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Absolute integrated line fluxes of H II regions have been measured using a Fabry-Perot spectrophotometer. We describe the observations and calibration procedures. Fluxes are given for 36 H II regions with Galactocentric distances ranging from 6.6 to 17.7 kpc. Several emission lines have been measured, mainly [O II] lambda lambda 3726 and 3629, H beta, [O III] lambda 5007, He I lambda 5876 and H alpha. The very faint [O III] lambda 4363 line has been measured in six regions, allowing a direct determination of the electron temperature. New photometric distances have been derived based on data from the literature. A discussion of these results in terms of extinction, electron density and temperature, and oxygen and helium abundances is given in Paper II.
引用
收藏
页码:317 / 328
页数:12
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