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Strong [O III] and [N II] emission lines in globular clusters from photoionized R Corona Borealis star winds
emission lines globular clusters
2011/1/13
The globular cluster X-ray source CXO J033831.8-352604 in NGC 1399 has recently been found to show strong emission lines of [O III] and [N II] in its optical spectrum in addition to ultraluminous X-ra...
Instabilities in Hot Star Winds。
Observations of Small-Scale Structure in AGB Star Winds:Precursors of Neutral Globules in PNE?
Small-Scale Structure Neutral Globules AGB Star Winds
2009/6/15
Observations of Small-Scale Structure in AGB Star Winds:Precursors of Neutral Globules in PNE?
Three-Component Modeling of C-Rich AGB Star Winds。