1. Stellar windA stellar wind is a flow of neutral or charged gas ejected from the upper atmosphere of a star. It is distinguished from the bipolar outflows characteristic of young stars by being less collimated, although stellar winds are not generally spherically symmetric. Different types of stars have different types of stellar winds. Post-main-sequence stars nearing the ends of their lives often eject large quantities of mass in massive (solar masses per year), slow winds.
Read “Stellar wind” on English Wikipedia
Read “恒星風” on Japanese Wikipedia
Read “Stellar wind” on DBpedia
Read “Stellar wind” on English Wikipedia
Read “恒星風” on Japanese Wikipedia
Read “Stellar wind” on DBpedia
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