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dbr:Betelgeuse	dbo:wikiPageWikiLink	dbr:Stellar_mass_loss .
<http://dbpedia.org/resource/Tolman\u2013Oppenheimer\u2013Volkoff_limit>	dbo:wikiPageWikiLink	dbr:Stellar_mass_loss .
dbr:R136a1	dbo:wikiPageWikiLink	dbr:Stellar_mass_loss .
dbr:Asymptotic_giant_branch	dbo:wikiPageWikiLink	dbr:Stellar_mass_loss .
@prefix foaf:	<http://xmlns.com/foaf/0.1/> .
@prefix wikipedia-en:	<http://en.wikipedia.org/wiki/> .
wikipedia-en:Stellar_mass_loss	foaf:primaryTopic	dbr:Stellar_mass_loss .
dbr:Star	dbo:wikiPageWikiLink	dbr:Stellar_mass_loss .
dbr:AFGL_2298	dbo:wikiPageWikiLink	dbr:Stellar_mass_loss .
<http://dbpedia.org/resource/Pleione_(star)>	dbo:wikiPageWikiLink	dbr:Stellar_mass_loss .
dbr:Heavy_metals	dbo:wikiPageWikiLink	dbr:Stellar_mass_loss .
dbr:Alpha_Herculis	dbo:wikiPageWikiLink	dbr:Stellar_mass_loss .
@prefix rdf:	<http://www.w3.org/1999/02/22-rdf-syntax-ns#> .
@prefix yago:	<http://dbpedia.org/class/yago/> .
dbr:Stellar_mass_loss	rdf:type	yago:Phenomenon100034213 ,
		yago:WikicatStellarPhenomena ,
		yago:PhysicalEntity100001930 ,
		dbo:Disease ,
		yago:Process100029677 .
@prefix rdfs:	<http://www.w3.org/2000/01/rdf-schema#> .
dbr:Stellar_mass_loss	rdfs:label	"\u6046\u661F\u8CEA\u91CF\u6D41\u5931"@zh ,
		"Perte de masse stellaire"@fr ,
		"Stellar mass loss"@en ,
		"P\u00E8rdua de massa estel\u00B7lar"@ca ,
		"\u041F\u043E\u0442\u0435\u0440\u044F \u043C\u0430\u0441\u0441\u044B \u0437\u0432\u0435\u0437\u0434\u043E\u0439"@ru ,
		"P\u00E9rdida de masa estelar"@es ;
	rdfs:comment	"Stellar mass loss is a phenomenon observed in stars. All stars lose some mass over their lives at widely varying rates. Triggering events can cause the sudden ejection of a large portion of the star's mass. Stellar mass loss can also occur when a star gradually loses material to a binary companion or into interstellar space."@en ,
		"\u6046\u661F\u8CEA\u91CF\u6D41\u5931\uFF08Stellar mass loss\uFF09\u662F\u5728\u4E00\u4E9B\u5927\u8CEA\u91CF\u6046\u661F\u4E0A\u89C0\u6E2C\u5230\u7684\u73FE\u8C61\uFF0C\u5728\u6B64\u4E00\u4E8B\u4EF6\u7684\u767C\u751F\u6A5F\u5236\u6703\u9020\u6210\u6046\u661F\u5927\u90E8\u5206\u7684\u8CEA\u91CF\u88AB\u62CB\u5C04\u51FA\u53BB\uFF1B\u6216\u662F\u5728\u806F\u661F\u7CFB\u7D71\u4E2D\u7684\u4E00\u9846\u6046\u661F\u8CEA\u91CF\u9010\u6F38\u6D41\u5931\u81F3\u5B83\u7684\u4F34\u661F\u6216\u662F\u661F\u969B\u7A7A\u9593\u4E2D\u3002"@zh ,
		"En astronom\u00EDa, la p\u00E9rdida de masa estelar es un fen\u00F3meno observado en algunas estrellas masivas. Tiene lugar cuando un acontecimiento desencadenante provoca la eyecci\u00F3n de una parte significativa de la masa estelar, o cuando existe una p\u00E9rdida gradual de material, bien hacia una compa\u00F1era binaria o bien hacia el espacio interestelar."@es ,
		"\u041F\u043E\u0442\u0435\u0440\u044F \u043C\u0430\u0441\u0441\u044B \u0437\u0432\u0435\u0437\u0434\u043E\u0439 (\u0430\u043D\u0433\u043B. Stellar mass loss) \u2014 \u044F\u0432\u043B\u0435\u043D\u0438\u0435, \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0435\u043C\u043E\u0435 \u0443 \u043D\u0435\u043A\u043E\u0442\u043E\u0440\u044B\u0445 \u043C\u0430\u0441\u0441\u0438\u0432\u043D\u044B\u0445 \u0437\u0432\u0451\u0437\u0434. \u041F\u0440\u043E\u0438\u0441\u0445\u043E\u0434\u0438\u0442 \u0432 \u0441\u043B\u0443\u0447\u0430\u0435, \u043A\u043E\u0433\u0434\u0430 \u043D\u0435\u043A\u043E\u0442\u043E\u0440\u044B\u0439 \u043C\u0435\u0445\u0430\u043D\u0438\u0437\u043C \u043F\u0440\u0438\u0432\u043E\u0434\u0438\u0442 \u043A \u0432\u044B\u0431\u0440\u043E\u0441\u0443 \u0437\u043D\u0430\u0447\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u043E\u043B\u0438\u0447\u0435\u0441\u0442\u0432\u0430 \u0432\u0435\u0449\u0435\u0441\u0442\u0432\u0430 \u0437\u0432\u0435\u0437\u0434\u044B. \u0422\u0430\u043A\u0436\u0435 \u0437\u0432\u0435\u0437\u0434\u0430 \u043C\u043E\u0436\u0435\u0442 \u0442\u0435\u0440\u044F\u0442\u044C \u043C\u0430\u0441\u0441\u0443 \u043F\u0440\u0438 \u043F\u043E\u0441\u0442\u0435\u043F\u0435\u043D\u043D\u043E\u043C \u043F\u0435\u0440\u0435\u0442\u0435\u043A\u0430\u043D\u0438\u0438 \u0432\u0435\u0449\u0435\u0441\u0442\u0432\u0430 \u043D\u0430 \u0432\u0442\u043E\u0440\u043E\u0439 \u043A\u043E\u043C\u043F\u043E\u043D\u0435\u043D\u0442 \u0432 \u0434\u0432\u043E\u0439\u043D\u043E\u0439 \u0441\u0438\u0441\u0442\u0435\u043C\u0435 \u0438\u043B\u0438 \u0432 \u043E\u043A\u0440\u0443\u0436\u0430\u044E\u0449\u0435\u0435 \u043F\u0440\u043E\u0441\u0442\u0440\u0430\u043D\u0441\u0442\u0432\u043E."@ru ,
		"La perte de masse stellaire est un ph\u00E9nom\u00E8ne observ\u00E9 chez certaines \u00E9toiles massives. Il se produit lorsqu'un \u00E9v\u00E9nement d\u00E9clencheur provoque l'\u00E9jection d'une importante quantit\u00E9 de masse de l'\u00E9toile, au profit d'une autre \u00E9toile dans un syst\u00E8me binaire, ou directement dans l'espace interstellaire."@fr ,
		"En astronomia, la p\u00E8rdua de massa estel\u00B7lar \u00E9s un fenomen observat en alguns estels massius. T\u00E9 lloc quan un esdeveniment desencadenant provoca l'ejecci\u00F3 d'una part significativa de la massa estel\u00B7lar, o quan existeix una p\u00E8rdua gradual de material, b\u00E9 cap a una companya bin\u00E0ria o b\u00E9 cap a l'espai interestel\u00B7lar."@ca .
@prefix dct:	<http://purl.org/dc/terms/> .
@prefix dbc:	<http://dbpedia.org/resource/Category:> .
dbr:Stellar_mass_loss	dct:subject	dbc:Stellar_phenomena ;
	dbo:abstract	"Stellar mass loss is a phenomenon observed in stars. All stars lose some mass over their lives at widely varying rates. Triggering events can cause the sudden ejection of a large portion of the star's mass. Stellar mass loss can also occur when a star gradually loses material to a binary companion or into interstellar space."@en ,
		"\u6046\u661F\u8CEA\u91CF\u6D41\u5931\uFF08Stellar mass loss\uFF09\u662F\u5728\u4E00\u4E9B\u5927\u8CEA\u91CF\u6046\u661F\u4E0A\u89C0\u6E2C\u5230\u7684\u73FE\u8C61\uFF0C\u5728\u6B64\u4E00\u4E8B\u4EF6\u7684\u767C\u751F\u6A5F\u5236\u6703\u9020\u6210\u6046\u661F\u5927\u90E8\u5206\u7684\u8CEA\u91CF\u88AB\u62CB\u5C04\u51FA\u53BB\uFF1B\u6216\u662F\u5728\u806F\u661F\u7CFB\u7D71\u4E2D\u7684\u4E00\u9846\u6046\u661F\u8CEA\u91CF\u9010\u6F38\u6D41\u5931\u81F3\u5B83\u7684\u4F34\u661F\u6216\u662F\u661F\u969B\u7A7A\u9593\u4E2D\u3002"@zh ,
		"\u041F\u043E\u0442\u0435\u0440\u044F \u043C\u0430\u0441\u0441\u044B \u0437\u0432\u0435\u0437\u0434\u043E\u0439 (\u0430\u043D\u0433\u043B. Stellar mass loss) \u2014 \u044F\u0432\u043B\u0435\u043D\u0438\u0435, \u043D\u0430\u0431\u043B\u044E\u0434\u0430\u0435\u043C\u043E\u0435 \u0443 \u043D\u0435\u043A\u043E\u0442\u043E\u0440\u044B\u0445 \u043C\u0430\u0441\u0441\u0438\u0432\u043D\u044B\u0445 \u0437\u0432\u0451\u0437\u0434. \u041F\u0440\u043E\u0438\u0441\u0445\u043E\u0434\u0438\u0442 \u0432 \u0441\u043B\u0443\u0447\u0430\u0435, \u043A\u043E\u0433\u0434\u0430 \u043D\u0435\u043A\u043E\u0442\u043E\u0440\u044B\u0439 \u043C\u0435\u0445\u0430\u043D\u0438\u0437\u043C \u043F\u0440\u0438\u0432\u043E\u0434\u0438\u0442 \u043A \u0432\u044B\u0431\u0440\u043E\u0441\u0443 \u0437\u043D\u0430\u0447\u0438\u0442\u0435\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u043E\u043B\u0438\u0447\u0435\u0441\u0442\u0432\u0430 \u0432\u0435\u0449\u0435\u0441\u0442\u0432\u0430 \u0437\u0432\u0435\u0437\u0434\u044B. \u0422\u0430\u043A\u0436\u0435 \u0437\u0432\u0435\u0437\u0434\u0430 \u043C\u043E\u0436\u0435\u0442 \u0442\u0435\u0440\u044F\u0442\u044C \u043C\u0430\u0441\u0441\u0443 \u043F\u0440\u0438 \u043F\u043E\u0441\u0442\u0435\u043F\u0435\u043D\u043D\u043E\u043C \u043F\u0435\u0440\u0435\u0442\u0435\u043A\u0430\u043D\u0438\u0438 \u0432\u0435\u0449\u0435\u0441\u0442\u0432\u0430 \u043D\u0430 \u0432\u0442\u043E\u0440\u043E\u0439 \u043A\u043E\u043C\u043F\u043E\u043D\u0435\u043D\u0442 \u0432 \u0434\u0432\u043E\u0439\u043D\u043E\u0439 \u0441\u0438\u0441\u0442\u0435\u043C\u0435 \u0438\u043B\u0438 \u0432 \u043E\u043A\u0440\u0443\u0436\u0430\u044E\u0449\u0435\u0435 \u043F\u0440\u043E\u0441\u0442\u0440\u0430\u043D\u0441\u0442\u0432\u043E."@ru ,
		"La perte de masse stellaire est un ph\u00E9nom\u00E8ne observ\u00E9 chez certaines \u00E9toiles massives. Il se produit lorsqu'un \u00E9v\u00E9nement d\u00E9clencheur provoque l'\u00E9jection d'une importante quantit\u00E9 de masse de l'\u00E9toile, au profit d'une autre \u00E9toile dans un syst\u00E8me binaire, ou directement dans l'espace interstellaire."@fr ,
		"En astronom\u00EDa, la p\u00E9rdida de masa estelar es un fen\u00F3meno observado en algunas estrellas masivas. Tiene lugar cuando un acontecimiento desencadenante provoca la eyecci\u00F3n de una parte significativa de la masa estelar, o cuando existe una p\u00E9rdida gradual de material, bien hacia una compa\u00F1era binaria o bien hacia el espacio interestelar."@es ,
		"En astronomia, la p\u00E8rdua de massa estel\u00B7lar \u00E9s un fenomen observat en alguns estels massius. T\u00E9 lloc quan un esdeveniment desencadenant provoca l'ejecci\u00F3 d'una part significativa de la massa estel\u00B7lar, o quan existeix una p\u00E8rdua gradual de material, b\u00E9 cap a una companya bin\u00E0ria o b\u00E9 cap a l'espai interestel\u00B7lar."@ca ;
	dbo:wikiPageWikiLink	dbr:Solar_flares ,
		dbr:Planetary_nebula ,
		dbc:Stellar_phenomena ,
		dbr:Solar_wind ,
		dbr:Coronal_mass_ejections ,
		dbr:Black_hole ,
		dbr:Star ,
		dbr:Binary_star ,
		dbr:Betelgeuse ,
		dbr:Stellar_evolution ,
		dbr:Helium_flash ,
		dbr:Wolf-Rayet_stars ,
		dbr:Sun ,
		dbr:White_dwarf ,
		dbr:Red_giant ,
		dbr:Coronal_mass_ejection ,
		dbr:Neutron_star ,
		dbr:Solar_mass ,
		dbr:Red_supergiant .
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dbr:X-ray_burster	dbo:wikiPageWikiLink	dbr:Stellar_mass_loss .
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