About: dbpedia:Spiral

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A spiral galaxy is a certain kind of galaxy originally described by Edwin Hubble in his 1936 work The Realm of the Nebulae and, as such, forms part of the Hubble sequence. Spiral galaxies consist of a flat, rotating disc containing stars, gas and dust, and a central concentration of stars known as the bulge.

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rdfs:comment	A spiral galaxy is a certain kind of galaxy originally described by Edwin Hubble in his 1936 work The Realm of the Nebulae and, as such, forms part of the Hubble sequence. Spiral galaxies consist of a flat, rotating disc containing stars, gas and dust, and a central concentration of stars known as the bulge.
rdfs:seeAlso	dbpedia:Density_wave_theory dbpedia:Gravitationally_aligned_orbits
foaf:depiction
thumbnail	http://en.wikipedia.org/wiki/Special:FilePath/M101_hires_STScI-PRC2006-10a.jpg?width=300
is rdfs:seeAlso of	dbpedia:Hubble_sequence
is type of	NGC 38 NGC634 NGC 41 NGC3938 NGC36,UGC106,PGC798,IRAS00088+0606, IRAS F00088+0606,CGCG408-040, CGCG 0008.8+0606,HIPASSJ0011+06,MCG+01-01-043, UZC J001122.3+062321, 2MASX J00112231+0623212,[HDL96]408-066,GC19 NGC 12 NGC 13 UGCA 002, ESO 472-G016, MCG -04-01-018, CGS 119,PGC701, ESO-LV 4720160 NGC 26 NGC 27 MCG-05-01-037, ESO 409-G022, AM 0005-301, PGC 627, h 4014, GC 2 UGC 9796 518, PGC 5161, UGC 952, MCG 1-4-49, ZWG 411.47 NGC 6560

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