基于W几何形的恒星光谱分子带检测
陈奋
1,
2
, 王颖
1,
2,
*
, 刘福窑
1,
2
Spectral Molecular Band Detection Based on W Geometry
CHEN Fen
1,
2
, WANG Ying
1,
2,
*
, LIU Fu-yao
1,
2
形状因子中V形整合示例图 (a)和(b)数据分别来自为LAMOST J093026.12+071221.0(obsid为805206193)和LAMOST J193205.73+402007.3(obsid为52803163)恒星光谱