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- T_Tauri_wind abstract "The T Tauri wind — so named because of the young star currently in this stage—is a phenomenon indicative of the phase of stellar development between the accretion of material from the slowing rotating material of a solar nebula and the ignition of the hydrogen that has agglomerated into the protostar.The protostar at first only has about 1% of its final mass. But the envelope of the star continues to grow as infalling material is accreted. After 10,000–100,000 years, thermonuclear fusion begins in its core, then a strong stellar wind is produced which stops the infall of new mass. The protostar is now considered a young star since its mass is fixed, and its future evolution is now set.".
- T_Tauri_wind wikiPageExternalLink index.html.
- T_Tauri_wind wikiPageExternalLink 1O80-TTauriwind.html.
- T_Tauri_wind wikiPageExternalLink abstract210.html.
- T_Tauri_wind wikiPageExternalLink solar_wind.html&edu=high.
- T_Tauri_wind wikiPageExternalLink lec13.html.
- T_Tauri_wind wikiPageID "11508745".
- T_Tauri_wind wikiPageLength "6088".
- T_Tauri_wind wikiPageOutDegree "13".
- T_Tauri_wind wikiPageRevisionID "653906484".
- T_Tauri_wind wikiPageWikiLink Astronomical_unit.
- T_Tauri_wind wikiPageWikiLink Category:Star_formation.
- T_Tauri_wind wikiPageWikiLink Category:T_Tauri_stars.
- T_Tauri_wind wikiPageWikiLink Formation_and_evolution_of_the_Solar_System.
- T_Tauri_wind wikiPageWikiLink Hydrogen.
- T_Tauri_wind wikiPageWikiLink Kelvin.
- T_Tauri_wind wikiPageWikiLink Magnetosphere.
- T_Tauri_wind wikiPageWikiLink Protoplanetary_disk.
- T_Tauri_wind wikiPageWikiLink Protostar.
- T_Tauri_wind wikiPageWikiLink Solar_nebula.
- T_Tauri_wind wikiPageWikiLink T_Tauri.
- T_Tauri_wind wikiPageWikiLink T_Tauri_star.
- T_Tauri_wind wikiPageWikiLink T_Tauri_stars.
- T_Tauri_wind wikiPageWikiLink Ultraviolet.
- T_Tauri_wind wikiPageWikiLinkText "T Tauri wind".
- T_Tauri_wind hasPhotoCollection T_Tauri_wind.
- T_Tauri_wind wikiPageUsesTemplate Template:Multiple_issues.
- T_Tauri_wind wikiPageUsesTemplate Template:Reflist.
- T_Tauri_wind subject Category:Star_formation.
- T_Tauri_wind subject Category:T_Tauri_stars.
- T_Tauri_wind type Article.
- T_Tauri_wind type Article.
- T_Tauri_wind type Page.
- T_Tauri_wind type Variable.
- T_Tauri_wind comment "The T Tauri wind — so named because of the young star currently in this stage—is a phenomenon indicative of the phase of stellar development between the accretion of material from the slowing rotating material of a solar nebula and the ignition of the hydrogen that has agglomerated into the protostar.The protostar at first only has about 1% of its final mass. But the envelope of the star continues to grow as infalling material is accreted.".
- T_Tauri_wind label "T Tauri wind".
- T_Tauri_wind sameAs m.02rg8fx.
- T_Tauri_wind sameAs Q7672683.
- T_Tauri_wind sameAs Q7672683.
- T_Tauri_wind sameAs 金牛T風.
- T_Tauri_wind wasDerivedFrom T_Tauri_wind?oldid=653906484.
- T_Tauri_wind isPrimaryTopicOf T_Tauri_wind.