BCD星系VII Zw 403（UGC 6456）中的气体和尘埃
Gas and dust in the BCD galaxy VII Zw 403 (UGC 6456)
摘要：
基于早期的光谱观测的结果与6米BTA望远镜的SAO RAS我们完善的金属丰度估计的复合物的电离气体在第七Zw 403星系。斯皮策太空望远镜的红外观测被用来寻找一个可能的相关性的多环芳烃（PAH）的质量分数分布的电离和中性氢的分布，并与气体的金属丰度在HII地区的星系。
英文摘要：
Based on the results of the earlier spectroscopic observations with the 6-m BTA telescope of the SAO RAS we refine the metallicity estimates of the complexes of ionized gas in the VII Zw 403 galaxy. Infrared observations from the Spitzer Space Telescope are used to search for a possible correlation of the mass fraction distribution of the polycyclic aromatic hydrocarbons (PAH) with the distribution of ionized and neutral hydrogen, and with the metallicity of gas in the HII regions of the galaxy.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
