Comparison of integrated photometric parameters of extragalactic star formation complexes and open star clusters in the Milky Way

被引：1
|
作者：
Gusev, A. S. [1 ]
Piskunov, A. E. [2 ]
Sakhibov, F. Kh. [3 ,4 ]
Kharchenko, N. V. [5 ]
机构：
[1] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119992, Russia
[2] Russian Acad Sci INASAN, Inst Astron, Moscow 119017, Russia
[3] Giessen Friedberg Univ Appl Sci, Friedberg, Germany
[4] Tajik Acad Sci, Inst Astrophys, Dushanbe 734042, Tajikistan
[5] Natl Acad Sci Ukraine, Main Astron Observ, UA-03680 Kiev, Ukraine
来源：
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2009年 / 35卷 / 10期
基金：
俄罗斯基础研究基金会;
关键词：
open star clusters; galaxies; H II regions; star-forming regions; interstellar extinction; LARGE-MAGELLANIC-CLOUD; GALACTIC OPEN CLUSTERS; INITIAL MASS FUNCTION; MULTICOLOR PHOTOMETRY; FORMING COMPLEXES; GALAXIES; EXTINCTION; REGIONS; ASSOCIATIONS; ULTRAVIOLET;
D O I：
10.1134/S1063773709100041
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A comparative analysis of the evolution of integrated photometric parameters for young star formation complexes in spiral and irregular galaxies and open star clusters in our Galaxy is performed. Extragalactic star formation complexes seen as giant H II regions and open star clusters in the Milky Way are shown to represent a single evolutionary sequence of objects at different stages of their evolution when the extinction is properly taken into account.
引用
收藏
页码：679 / 687
页数：9
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