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- HD_206267 abstract "HD 206267 is a triple star. It lies in the nebula IC 1396. All three components are large and powerful blue stars, and the intense ultraviolet radiation they give off ionizes the gas of IC 1396, and causes compression denser globules of the nebula, leading to star formation. The stellar wind produced by the stars is strong enough to strip nearby stars of their protoplanetary disks.".
- HD_206267 wikiPageExternalLink hd-206267.shtml.
- HD_206267 wikiPageID "16718262".
- HD_206267 wikiPageRevisionID "599633046".
- HD_206267 absmagV "5.83".
- HD_206267 age "3000000".
- HD_206267 appmagV "5.28".
- HD_206267 class "O6V+O9V".
- HD_206267 constell Cepheus_(constellation).
- HD_206267 epoch "J2000".
- HD_206267 hasPhotoCollection HD_206267.
- HD_206267 mass "23".
- HD_206267 pError "0.79".
- HD_206267 parallax "2.78".
- HD_206267 propMoDec "-5.04".
- HD_206267 propMoRa "-1.71".
- HD_206267 radialV "-7.8".
- HD_206267 variable "None".
- HD_206267 subject Category:Cepheus_(constellation).
- HD_206267 subject Category:HR_objects.
- HD_206267 subject Category:Henry_Draper_Catalogue_objects.
- HD_206267 type CelestialBody.
- HD_206267 type Star.
- HD_206267 type PhysicalBody.
- HD_206267 comment "HD 206267 is a triple star. It lies in the nebula IC 1396. All three components are large and powerful blue stars, and the intense ultraviolet radiation they give off ionizes the gas of IC 1396, and causes compression denser globules of the nebula, leading to star formation. The stellar wind produced by the stars is strong enough to strip nearby stars of their protoplanetary disks.".
- HD_206267 label "HD 206267".
- HD_206267 label "螣蛇七".
- HD_206267 sameAs m.04043dd.
- HD_206267 sameAs Q5097827.
- HD_206267 sameAs Q5097827.
- HD_206267 wasDerivedFrom HD_206267?oldid=599633046.
- HD_206267 isPrimaryTopicOf HD_206267.
- HD_206267 name "HD 206267A1".