The Radial Oxygen Abundance Gradient from OB Stars in the Outer Galactic Disk

Astronomical Society of the Pacific Conference Series(2019)

引用 0|浏览24
暂无评分
摘要
Metallicity gradients are important constraints for models of chemical evolution of the Galaxy. We present the current radial gradient of oxygen abundances using a sample of main -sequence OB stars located in the outer Galactic Disk, considering non-NLTE abundances, and distances based on GAIA DR2 results. We compare the obtained gradient with results from other young objects of the Galactic Disk.
更多
查看译文
AI 理解论文
溯源树
样例
生成溯源树,研究论文发展脉络
Chat Paper
正在生成论文摘要