论文标题
S0 Galaxy NGC 4324的环中的年轻恒星形成复合物
Young Star-Forming Complexes in the Ring of the S0 galaxy NGC 4324
论文作者
论文摘要
我们介绍了我们研究的研究结果的结果。 - 我们已经检测到位于凸状星系NGC 4324内环中的年轻星形配合物（团块），我们已经建立了它们沿环的规则分布模式，尽管如此，随着时间的变化（随着时间的时间而变化）。我们建议凸状星系NGC 4324的几个可能的进化路径，其中最有可能的是富含气体的卫星或巨型云（所谓的小型合并）。
We present the results of our study of starforming regions in the lenticular galaxy NGC 4324. During a complex analysis of multiwavelength observational data -- the narrow-band emission-line images obtained with the 2.5-m telescope at the Caucasus Mountain Observatory of the Sternberg Astronomical Institute of the Moscow State University and the archival images in the broad bands of the SDSS, GALEX and WISE surveys -- we have detected young starforming complexes (clumps) located in the inner ring of the lenticular galaxy NGC 4324, and we have established a regular pattern of their distribution along the ring, which, nevertheless, changes with time (with age of starforming regions). We suggest several possible evolutionary paths of the lenticular galaxy NGC 4324, of which the accretion of gas-rich satellites or giant clouds (the so-called minor merging) is the most probable one.
