PMO OpenIR  > 星系中的恒星形成研究团组
恒星形成区AFGL 5157的CO同位素分子谱线研究
毛春花 ; 杨戟 ; 逯登荣
2013
Source Publication天文学报
ISSN0001-5245
Volume54Issue:4Pages:365-317
Abstract与国家天文台兴隆站2.16 m安装的北京天文台暗天体分光成像仪(BAO FaintObject Spectrograph and Camera,BFOSC)系统相似,云南天文台2.4 m望远镜安装了云南暗弱天体光谱及成像仪(Yunnan Faint-Object Spectrograph and Camera,YFOSC),对它在直接照相时的CCD平场性能做了测定。使用不同旋转角度拍摄平均而得的平场,可以使不同位置拍摄的像场,所受最大误差≤0.015 mag。但与卡焦的VersArray CCD照相机不同,即使在视场中间直径6.'5的圆内,误差约在0.010~0.013 mag之间,达不到≤0.005 mag的精度。
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/9883
Collection星系中的恒星形成研究团组
Recommended Citation
GB/T 7714
毛春花,杨戟,逯登荣. 恒星形成区AFGL 5157的CO同位素分子谱线研究[J]. 天文学报,2013,54(4):365-317.
APA 毛春花,杨戟,&逯登荣.(2013).恒星形成区AFGL 5157的CO同位素分子谱线研究.天文学报,54(4),365-317.
MLA 毛春花,et al."恒星形成区AFGL 5157的CO同位素分子谱线研究".天文学报 54.4(2013):365-317.
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