Distributions, equivalent widths and metallicities of the HII regions in the spiral galaxies NGC 5457 and NGC 4395

被引：36

作者：

Cedrés, B ^{[1
]}

Cepa, J

机构：

[1] Inst Astrofis Canarias, Tenerife 38205, Spain

[2] Univ La Laguna, Fac Fis, Dept Astrofis, Tenerife 38071, Spain

来源：

ASTRONOMY & ASTROPHYSICS | 2002年 / 391卷 / 03期

关键词：

HII regions; galaxies; individual; NGC; 4395; 5194; galaxies : abundances;

D O I：

10.1051/0004-6361:20020588

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Using CCD observations in the narrow band filters in Halpha, Hbeta,[O II], [O III], [S II] and [S III] lines we have compiled a catalogue of 338 H regions for the inner parts of NGC 5457 and 158 for NGC 4395. The extinction, equivalent widths, distributions, excitations, ionization hardness, ionization parameters and metallicities for these regions, a distinction being made between arm and inter-arm zones, are presented here with the first results of a study of stellar formation.

引用

页码：809 / 821

页数：13

共 31 条

[21] The O/H distribution in the low-mass galaxies NGC 2366 and NGC 4395 [J].