Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q917926> ?p ?o }
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- Q917926 subject Q1031119.
- Q917926 subject Q10596.
- Q917926 subject Q7152546.
- Q917926 subject Q7152550.
- Q917926 subject Q7282683.
- Q917926 abstract "NGC 4319 is a face-on barred spiral galaxy located about 77 million light years away in the constellation Draco. The morphological classification is SB(r)ab, which indicates it is a barred spiral with an inner ring structure and moderate to tightly wound arms. It is situated in physical proximity to the galaxies NGC 4291 and NGC 4386, with X-ray emissions from the intervening gap indicating NGC 4319 and NGC 4291 may be interacting. NGC 4319 has a much higher proportion of ionized hydrogen compared to the Milky Way galaxy.In 1971, American astronomer Halton Arp noted what appeared to be a physical connection between NGC 4319 and Markarian 205, a quasi-stellar object with a much higher redshift. He suggested that if Markarian 205 is not an accidentally projected background object, then it may instead have been ejected from the nucleus of this galaxy. The discovery of an apparent luminous connection between the two created a storm of controversy as astronomers sought to refute the assertion and provide other explanations. The matter was effectively settled when observations using the Hubble Space Telescope showed that the light from Markarian 205 was passing through the disk and halo of NGC 4319 to reach the observer, placing Markarian 205 behind this galaxy and thus further away.".
- Q917926 thumbnail NGC_4319_I_HST2002.jpg?width=300.
- Q917926 wikiPageExternalLink fast_facts.html.
- Q917926 wikiPageExternalLink supplemental.html.
- Q917926 wikiPageWikiLink Q1031119.
- Q917926 wikiPageWikiLink Q10596.
- Q917926 wikiPageWikiLink Q12129.
- Q917926 wikiPageWikiLink Q14534.
- Q917926 wikiPageWikiLink Q1479861.
- Q917926 wikiPageWikiLink Q182429.
- Q917926 wikiPageWikiLink Q1852.
- Q917926 wikiPageWikiLink Q23548.
- Q917926 wikiPageWikiLink Q2490.
- Q917926 wikiPageWikiLink Q2513.
- Q917926 wikiPageWikiLink Q2703.
- Q917926 wikiPageWikiLink Q321.
- Q917926 wikiPageWikiLink Q42262.
- Q917926 wikiPageWikiLink Q453729.
- Q917926 wikiPageWikiLink Q531.
- Q917926 wikiPageWikiLink Q615925.
- Q917926 wikiPageWikiLink Q631379.
- Q917926 wikiPageWikiLink Q644507.
- Q917926 wikiPageWikiLink Q7152546.
- Q917926 wikiPageWikiLink Q7152550.
- Q917926 wikiPageWikiLink Q7282683.
- Q917926 wikiPageWikiLink Q76250.
- Q917926 wikiPageWikiLink Q83373.
- Q917926 wikiPageWikiLink Q8675.
- Q917926 wikiPageWikiLink Q8928.
- Q917926 wikiPageWikiLink Q917926.
- Q917926 name "NGC 4319".
- Q917926 names "UGC 7429, PGC 39981".
- Q917926 type Place.
- Q917926 type CelestialBody.
- Q917926 type Galaxy.
- Q917926 type Location.
- Q917926 type Place.
- Q917926 type Thing.
- Q917926 type Q318.
- Q917926 comment "NGC 4319 is a face-on barred spiral galaxy located about 77 million light years away in the constellation Draco. The morphological classification is SB(r)ab, which indicates it is a barred spiral with an inner ring structure and moderate to tightly wound arms. It is situated in physical proximity to the galaxies NGC 4291 and NGC 4386, with X-ray emissions from the intervening gap indicating NGC 4319 and NGC 4291 may be interacting.".
- Q917926 label "NGC 4319".
- Q917926 depiction NGC_4319_I_HST2002.jpg.
- Q917926 name "NGC4319".
- Q917926 name "UGC7429,PGC39981".