Star Formation in Nearby Dwarf Galaxies

被引：8

作者：

Kaisin, S. S. ^{[1
]}

Karachentsev, I. D. ^{[1
]}

机构：

[1] Russian Acad Sci, Special Astrophys Observ, Nizhnii Arkhyz 369167, Russia

来源：

ASTROPHYSICAL BULLETIN | 2019年 / 74卷 / 01期

基金：

俄罗斯科学基金会;

关键词：

galaxies: dwarf; galaxies: star formation; H-ALPHA; DATABASE; SAMPLE; LIST;

D O I：

10.1134/S1990341319010012

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report the measured H fluxes and images of 66 nearby objects observed with the 6-m telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences. Three of these objectsIC 2233, UGC4704, and NGC3432are late-type spiral galaxies, six objects are distant globular clusters of the M31 galaxy, and the remaining ones are dwarf galaxies. We used the measured H fluxes to estimate the integrated and specific star-formation rates and analyzed some of the main features of star formation in dwarf galaxies and late-type spirals based on a sample of more than 500 Local-volume galaxies.

引用

页码：1 / 11

页数：11

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