摘要
对于大质量星的形成,由于区域的遥远和结构的复杂以及过程的特殊,研究相对迟缓.对可能形成大质量星的云核和大质量年轻星体的活动,进行了多波段搜寻和研究.取得了相应的进展.
Massive star formation regions are usually more distant from us and more compleax than low mass ones. Massive young stellar objects generally ionize the environment material in a short period. These lead to much less progress on their studies. With multiple wavebands, our group has been investigating massive cores where massive stars may be in forming process and activites of massive young stellar objects. Our work in this aspect is presented.
出处
《天文学进展》
CSCD
北大核心
2001年第2期246-248,共3页
Progress In Astronomy