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Statements

Subject Item
dbr:Ring_Nebula_(NGC_6822)
rdf:type
yago:PhysicalEntity100001930 yago:YagoGeoEntity yago:YagoLegalActorGeo yago:Location100027167 yago:YagoPermanentlyLocatedEntity yago:WikicatHIIRegions yago:Region108630039 yago:Object100002684
rdfs:label
Ring Nebula (NGC 6822) 環狀星雲 (NGC 6822)
rdfs:comment
在巴納德星系中的環狀星雲官方正式的名稱是Hubble 1925 III(羅馬數字的3)，當時他首度被記錄在哈伯1925年的論文：N.G.C. 6822, A Remote Stellar System。它包含一個明亮的電離氫區發射。在1977年的論文中它被註記為Hodge 4。 它的外觀與在大麥哲倫星系內發現的絲狀星雲非常相似 (參見Meaburn 1981)；它最類似於LMC中的圓環形星雲N70。 The Ring Nebula in Barnard's Galaxy has the official designation of Hubble 1925 III as it was the third (Roman numeral 3) object recorded in Hubble's 1925 paper, N.G.C. 6822, A Remote Stellar System. It includes areas of bright H II emission. In Paul W. Hodge's 1977 paper it was designated Hodge 4. Its appearance is very similar to the filamentary nebula found in the Large Magellanic Cloud (see Meaburn 1981). It most resembles the circular ring-like nebula N70 in the LMC. In 1987 this object Hubble III in NGC 6822, was observed with the Manchester Echelle Spectrometer II.
dbp:name
Ring Nebula in Barnard's Galaxy
foaf:depiction
n8:NGC_6822_Bubble_and_Ring_nebulae.jpg
dcterms:subject
dbc:H_II_regions dbc:NGC_6822 dbc:Sagittarius_(constellation)
dbo:wikiPageID
5848020
dbo:wikiPageRevisionID
1085858125
dbo:wikiPageWikiLink
dbr:H_II_region dbr:Monthly_Notices_of_the_Royal_Astronomical_Society dbr:Lyon-Meudon_Extragalactic_Database dbr:New_General_Catalogue dbr:Sagittarius_(constellation) dbr:Index_Catalogue dbc:H_II_regions dbr:IRAS dbc:Sagittarius_(constellation) dbr:Large_Magellanic_Cloud dbr:David_Dunlap_Observatory_Catalogue dbr:1_E22_m dbr:Bubble_Nebula_(NGC_6822) dbr:HIPASS dbc:NGC_6822 dbr:La_Silla_Observatory dbr:NGC_6822 dbr:Edwin_Hubble dbr:Parsec dbr:Barnard's_Galaxy dbr:Morphological_Catalogue_of_Galaxies dbr:Paul_W._Hodge
dbo:wikiPageExternalLink
n16:sim-basic%3FIdent=ngc+6822&submit=SIMBAD+search n17:1987MNRAS.226..493C
owl:sameAs
dbpedia-zh:環狀星雲_(NGC_6822) wikidata:Q4817159 dbpedia-tr:Halka_Bulutsusu_(NGC_6822) n20:4SwZd freebase:m.0f8vx1
dbp:sizeV
53
dbp:wikiPageUsesTemplate
dbt:Infobox_nebula dbt:For dbt:More_citations_needed dbt:Convert dbt:Reflist dbt:Nebula-stub
dbo:thumbnail
n8:NGC_6822_Bubble_and_Ring_nebulae.jpg?width=300
dbp:constellation
dbr:Sagittarius_(constellation)
dbp:distLy
1630000
dbp:appmagV
~14.5
dbp:caption
The Ring Nebula seen with the Bubble Nebula as taken at the La Silla Observatory
dbp:distPc
0.5
dbp:epoch
J2000.0
dbp:names
Hubble 1925 III, Hodge 4, NGC 6822B, NGC 6822-2, IRAS 19421-1455, DDO 209, LEDA 63616, HIPASS J1944-14, 2MASX J19445619-1447512, IC 4895, MCG-02-50-006
dbp:type
H II region
dbo:abstract
在巴納德星系中的環狀星雲官方正式的名稱是Hubble 1925 III(羅馬數字的3)，當時他首度被記錄在哈伯1925年的論文：N.G.C. 6822, A Remote Stellar System。它包含一個明亮的電離氫區發射。在1977年的論文中它被註記為Hodge 4。 它的外觀與在大麥哲倫星系內發現的絲狀星雲非常相似 (參見Meaburn 1981)；它最類似於LMC中的圓環形星雲N70。 The Ring Nebula in Barnard's Galaxy has the official designation of Hubble 1925 III as it was the third (Roman numeral 3) object recorded in Hubble's 1925 paper, N.G.C. 6822, A Remote Stellar System. It includes areas of bright H II emission. In Paul W. Hodge's 1977 paper it was designated Hodge 4. Its appearance is very similar to the filamentary nebula found in the Large Magellanic Cloud (see Meaburn 1981). It most resembles the circular ring-like nebula N70 in the LMC. In 1987 this object Hubble III in NGC 6822, was observed with the Manchester Echelle Spectrometer II.
dbp:dec
-14
dbp:ra
71076.0
dbp:radiusLy
~
prov:wasDerivedFrom
wikipedia-en:Ring_Nebula_(NGC_6822)?oldid=1085858125&ns=0
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2682
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wikipedia-en:Ring_Nebula_(NGC_6822)