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A giant star that exploded 30 million years ago in a galaxy near Earth had a radius prior to going supernova that was 200 times larger than our sun, according to astrophysicists at Southern Methodist ...
The softness parameter is based on the relative intensity of several optical emission lines emitted by the gas ionized by young massive star clusters and can be used to derive the equivalent effective...
VLT spectroscopy of massive stars in NGC55。
Wind-Blown Bubbles around Massive Stars. The effects of stellar wind and photo-ionization on the circumstellar Medium。
Massive Stars in Clusters and the Field。
Feedback Processes in Massive Star Formation。
Massive Stars in Transition:Spectroscopic Analysis of HR Carinae
Massive Star Formation Near the Supernova Remnant W30。

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