About: SSPSF model

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Astronomical theory that star formation propagates via the action of shock waves produced by stellar winds and supernovae traversing the gas that composes the interstellar medium

Property	Value
dbo:description	astronomical theory that star formation propagates via the action of shock waves produced by stellar winds and supernovae traversing the gas that composes the interstellar medium (en)
dbo:thumbnail	wiki-commons:Special:FilePath/Henize_206_(PIA05517).jpg?width=300
dbo:wikiPageWikiLink	dbr:Differential_rotation dbr:Spiral_galaxy dbr:Conway's_Game_of_Life dbr:NGC_4414 dbr:Disc_galaxy dbr:Stellar_wind dbr:Galaxy dbr:Grand_design_spiral_galaxy dbr:Spore_(2008_video_game) dbr:Density_wave_theory dbc:Star_formation dbr:Flocculent_spiral_galaxy dbr:Star_formation dbr:Interstellar_medium dbr:Cellular_automaton dbr:Supernova_remnant dbr:Compartmental_models_in_epidemiology dbr:Henize_206 dbr:Supernovae dbr:Irregular_galaxies dbr:Elliptical_galaxies dbr:File:SSPSF_simulation.gif
dbp:wikiPageUsesTemplate	dbt:Authority_control dbt:Reflist dbt:Annotated_link dbt:Short_description
dct:subject	dbc:Star_formation
rdfs:label	SSPSF model (en)
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prov:wasDerivedFrom	wikipedia-en:SSPSF_model?oldid=1283937472&ns=0
foaf:depiction	wiki-commons:Special:FilePath/NGC_4414_(NASA-med).jpg wiki-commons:Special:FilePath/SSPSF_simulation.gif wiki-commons:Special:FilePath/Henize_206_(PIA05517).jpg
foaf:isPrimaryTopicOf	wikipedia-en:SSPSF_model
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