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To understand how systems of star clusters have reached their presently observed properties constitutes a powerful probe into the physics of cluster formation, without needing to resort to high spatia...
We present near-infrared JHKs imaging as well as K-band multi-object spectroscopy of the massive stellar content of W3 Main using LUCI at the LBT. We confirm 13 OB stars by their absorption line spect...
Hii regions in ngc 5055. ii. physical properties     Hii regions  ngc 5055  physical properties       font style='font-size:12px;'> 2009/7/10
Hii regions in ngc 5055. ii. physical properties
The nature of the very extended emission line regions associated with active galactic nuclei
Iso spectroscopy of ultracompact H II regions:element abundance gradient in the galaxy。
Chemical Diffusion in Stellar Convective Regions     Chemical Diffusion  Stellar Convective Regions       font style='font-size:12px;'> 2009/6/10
Chemical Diffusion in Stellar Convective Regions
Density bounded H II regionsionization of the diffuse interstellar and intergalactic media。
Effects of the stellar component on derived physical parameters of galactic H II regions
Cloudy 94 and applications to quasar emission line regions     quasar emission line regions  Cloudy 94       font style='font-size:12px;'> 2009/6/5
Cloudy 94 and applications to quasar emission line regions

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