Browse Wiki & Semantic Web

Jump to: navigation, search
Http://dbpedia.org/resource/Westerhout 43
  This page has no properties.
hide properties that link here 
  No properties link to this page.
 
http://dbpedia.org/resource/Westerhout_43
http://dbpedia.org/ontology/abstract W43, también conocida cómo Westerhout 43 eW43, también conocida cómo Westerhout 43 es una región de formación estelar de nuestra galaxia situada en la constelación del Águila a una distancia estimada de 6 kiloparsecs del Sol, considerada cómo la zona de la Vía Láctea en la que se forman estrellas de modo más activo conocida.​ Se ubica en el conocido cómo Anillo 5 kiloparsecs, un anillo de hidrógeno molecular que rodea la barra central de la Vía Láctea y que se considera alberga buena parte de la formación estelar de ésta.​ y está tan oscurecida por el polvo interestelar que es totalmente invisible en el óptico y sólo puede estudiarse mediante longitudes de onda que penetran éste cómo el infrarrojo o las ondas de radio.​ cómo el infrarrojo o las ondas de radio.​ , Westerhout 43, também conhecida como W43, Westerhout 43, também conhecida como W43, é uma região de formação de estrelas da nossa galáxia localizada na constelação de Aquila, a uma distância de 6 quiloparsecs (cerca de 20.000 anos-luz ) do Sol, que é considerada a região da Via Láctea que mais ativamente forma estrelas. Apesar disso, porém, é tão fortemente obscurecida pela poeira interestelar que é totalmente invisível no espectro da luz visível e deve ser estudada usando outros comprimentos de onda que não são afetados por ela, como o infravermelho ou as ondas de rádio.como o infravermelho ou as ondas de rádio. , Westerhout 43, also known as W43, is a regWesterhout 43, also known as W43, is a region of star formation of our galaxy located in the constellation of Aquila at a distance of 6 kilo-parsecs (nearly 20,000 light-years) of the Sun, that is considered the region of the Milky Way that is most actively forming stars. Despite this, however, it is so heavily obscured by the interstellar dust that it is totally invisible in the optical and must be studied using other wavelengths that are not affected by it, such as the infrared or the radio waves., such as the infrared or the radio waves.
http://dbpedia.org/ontology/thumbnail http://commons.wikimedia.org/wiki/Special:FilePath/Image_of_the_W43_star-forming_region_from_the_Spitzer_Space_Telescope.jpg?width=300 +
http://dbpedia.org/ontology/wikiPageID 37979088
http://dbpedia.org/ontology/wikiPageLength 5274
http://dbpedia.org/ontology/wikiPageRevisionID 1118034616
http://dbpedia.org/ontology/wikiPageWikiLink http://dbpedia.org/resource/Molecular_hydrogen + , http://dbpedia.org/resource/Aquila_%28constellation%29 + , http://dbpedia.org/resource/Category:Aquila_%28constellation%29 + , http://dbpedia.org/resource/Infrared + , http://dbpedia.org/resource/Kilo- + , http://dbpedia.org/resource/Category:Emission_nebulae + , http://dbpedia.org/resource/Wavelength + , http://dbpedia.org/resource/NGC_3603 + , http://dbpedia.org/resource/Category:Star-forming_regions + , http://dbpedia.org/resource/Extinction_%28astronomy%29 + , http://dbpedia.org/resource/Interstellar_dust + , http://dbpedia.org/resource/Wolf-Rayet_star + , http://dbpedia.org/resource/O_star + , http://dbpedia.org/resource/Light-year + , http://dbpedia.org/resource/Barred_spiral_galaxy + , http://dbpedia.org/resource/Constellation + , http://dbpedia.org/resource/Visible_light + , http://dbpedia.org/resource/Milky_Way + , http://dbpedia.org/resource/R136 + , http://dbpedia.org/resource/Sun + , http://dbpedia.org/resource/Star_formation + , http://dbpedia.org/resource/Star_clusters + , http://dbpedia.org/resource/J2000 + , http://dbpedia.org/resource/Parsec + , http://dbpedia.org/resource/Molecular_cloud + , http://dbpedia.org/resource/Protostar + , http://dbpedia.org/resource/Large_Magellanic_Cloud + , http://dbpedia.org/resource/File:Image_of_the_W43_star-forming_region_from_the_Spitzer_Space_Telescope.jpg + , http://dbpedia.org/resource/Solar_mass + , http://dbpedia.org/resource/Starburst_galaxy + , http://dbpedia.org/resource/Radio_waves +
http://dbpedia.org/property/constellation http://dbpedia.org/resource/Aquila_%28constellation%29 +
http://dbpedia.org/property/epoch http://dbpedia.org/resource/J2000 +
http://dbpedia.org/property/name Westerhout 43
http://dbpedia.org/property/names SNR G030.8-00.0, 3C 390.2
http://dbpedia.org/property/sizeV 6.3
http://dbpedia.org/property/type molecular cloud
http://dbpedia.org/property/wikiPageUsesTemplate http://dbpedia.org/resource/Template:Infobox_nebula + , http://dbpedia.org/resource/Template:Aquila_%28constellation%29 + , http://dbpedia.org/resource/Template:Reflist + , http://dbpedia.org/resource/Template:Short_description + , http://dbpedia.org/resource/Template:DEC + , http://dbpedia.org/resource/Template:RA + , http://dbpedia.org/resource/Template:Val +
http://purl.org/dc/terms/subject http://dbpedia.org/resource/Category:Emission_nebulae + , http://dbpedia.org/resource/Category:Star-forming_regions + , http://dbpedia.org/resource/Category:Aquila_%28constellation%29 +
http://purl.org/linguistics/gold/hypernym http://dbpedia.org/resource/Region +
http://www.w3.org/ns/prov#wasDerivedFrom http://en.wikipedia.org/wiki/Westerhout_43?oldid=1118034616&ns=0 +
http://xmlns.com/foaf/0.1/depiction http://commons.wikimedia.org/wiki/Special:FilePath/Image_of_the_W43_star-forming_region_from_the_Spitzer_Space_Telescope.jpg +
http://xmlns.com/foaf/0.1/isPrimaryTopicOf http://en.wikipedia.org/wiki/Westerhout_43 +
owl:sameAs http://es.dbpedia.org/resource/Westerhout_43 + , http://www.wikidata.org/entity/Q5096732 + , http://dbpedia.org/resource/Westerhout_43 + , https://global.dbpedia.org/id/4iBqM + , http://rdf.freebase.com/ns/m.0pb4dr9 + , http://yago-knowledge.org/resource/Westerhout_43 + , http://pt.dbpedia.org/resource/Westerhout_43 +
rdf:type http://dbpedia.org/class/yago/WikicatEmissionNebulae + , http://dbpedia.org/class/yago/Compound114818238 + , http://dbpedia.org/class/yago/Chemical114806838 + , http://dbpedia.org/class/yago/Substance100019613 + , http://dbpedia.org/class/yago/PhysicalEntity100001930 + , http://dbpedia.org/class/yago/Matter100020827 + , http://dbpedia.org/class/yago/Material114580897 + , http://dbpedia.org/class/yago/Formulation114873641 + , http://dbpedia.org/ontology/Settlement + , http://dbpedia.org/class/yago/Relation100031921 + , http://dbpedia.org/class/yago/Part113809207 + , http://dbpedia.org/class/yago/Nebula114960606 + , http://dbpedia.org/class/yago/Abstraction100002137 +
rdfs:comment Westerhout 43, também conhecida como W43, Westerhout 43, também conhecida como W43, é uma região de formação de estrelas da nossa galáxia localizada na constelação de Aquila, a uma distância de 6 quiloparsecs (cerca de 20.000 anos-luz ) do Sol, que é considerada a região da Via Láctea que mais ativamente forma estrelas. Apesar disso, porém, é tão fortemente obscurecida pela poeira interestelar que é totalmente invisível no espectro da luz visível e deve ser estudada usando outros comprimentos de onda que não são afetados por ela, como o infravermelho ou as ondas de rádio.como o infravermelho ou as ondas de rádio. , Westerhout 43, also known as W43, is a regWesterhout 43, also known as W43, is a region of star formation of our galaxy located in the constellation of Aquila at a distance of 6 kilo-parsecs (nearly 20,000 light-years) of the Sun, that is considered the region of the Milky Way that is most actively forming stars. Despite this, however, it is so heavily obscured by the interstellar dust that it is totally invisible in the optical and must be studied using other wavelengths that are not affected by it, such as the infrared or the radio waves., such as the infrared or the radio waves. , W43, también conocida cómo Westerhout 43 eW43, también conocida cómo Westerhout 43 es una región de formación estelar de nuestra galaxia situada en la constelación del Águila a una distancia estimada de 6 kiloparsecs del Sol, considerada cómo la zona de la Vía Láctea en la que se forman estrellas de modo más activo conocida.​ Se ubica en el conocido cómo Anillo 5 kiloparsecs, un anillo de hidrógeno molecular que rodea la barra central de la Vía Láctea y que se considera alberga buena parte de la formación estelar de ésta.​ y está tan oscurecida por el polvo interestelar que es totalmente invisible en el óptico y sólo puede estudiarse mediante longitudes de onda que penetran éste cómo el infrarrojo o las ondas de radio.​ cómo el infrarrojo o las ondas de radio.​
rdfs:label Westerhout 43
hide properties that link here 
http://dbpedia.org/resource/List_of_star-forming_regions_in_the_Local_Group + , http://dbpedia.org/resource/Westerhout + http://dbpedia.org/ontology/wikiPageWikiLink
http://en.wikipedia.org/wiki/Westerhout_43 + http://xmlns.com/foaf/0.1/primaryTopic
http://dbpedia.org/resource/Westerhout_43 + owl:sameAs
 

 

Enter the name of the page to start semantic browsing from.