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- HL_Tau_76 abstract "HL Tau 76 is a variable white dwarf star of the DAV (or ZZ Ceti) type. It was observed by G. Haro and W. J. Luyten in 1961, and was the first variable white dwarf discovered when, in 1968, Arlo U. Landolt found that it varied in brightness with a period of approximately 749.5 seconds, or 12.5 minutes. Like other DAV white dwarfs, its variability arises from non-radial gravity wave pulsations within itself., § 7. Later observation and analysis has found HL Tau 76 to pulsate in over 40 independent vibrational modes, with periods between 380 seconds and 1390 seconds.".
- HL_Tau_76 wikiPageID "11335038".
- HL_Tau_76 wikiPageLength "3655".
- HL_Tau_76 wikiPageOutDegree "18".
- HL_Tau_76 wikiPageRevisionID "632782679".
- HL_Tau_76 wikiPageWikiLink Arlo_U._Landolt.
- HL_Tau_76 wikiPageWikiLink Category:Objects_named_with_variable_star_designations.
- HL_Tau_76 wikiPageWikiLink Category:Pulsating_white_dwarfs.
- HL_Tau_76 wikiPageWikiLink Category:Taurus_(constellation).
- HL_Tau_76 wikiPageWikiLink Epoch_(astronomy).
- HL_Tau_76 wikiPageWikiLink G._Haro.
- HL_Tau_76 wikiPageWikiLink Gravity_wave.
- HL_Tau_76 wikiPageWikiLink Guillermo_Haro.
- HL_Tau_76 wikiPageWikiLink International_Celestial_Reference_System.
- HL_Tau_76 wikiPageWikiLink J2000.0.
- HL_Tau_76 wikiPageWikiLink Normal_mode.
- HL_Tau_76 wikiPageWikiLink Pulsating_white_dwarf.
- HL_Tau_76 wikiPageWikiLink Second.
- HL_Tau_76 wikiPageWikiLink Star.
- HL_Tau_76 wikiPageWikiLink Taurus_(constellation).
- HL_Tau_76 wikiPageWikiLink Variable_star.
- HL_Tau_76 wikiPageWikiLink Vibrational_mode.
- HL_Tau_76 wikiPageWikiLink W._J._Luyten.
- HL_Tau_76 wikiPageWikiLink White_dwarf.
- HL_Tau_76 wikiPageWikiLink Willem_Jacob_Luyten.
- HL_Tau_76 wikiPageWikiLinkText "HL Tau 76".
- HL_Tau_76 appmagV "14.1".
- HL_Tau_76 bV "0.2".
- HL_Tau_76 class "DAV5".
- HL_Tau_76 constell Taurus_(constellation).
- HL_Tau_76 epoch "J2000.0".
- HL_Tau_76 hasPhotoCollection HL_Tau_76.
- HL_Tau_76 propMoDec "−72".
- HL_Tau_76 propMoRa "66".
- HL_Tau_76 variable "DAV".
- HL_Tau_76 wikiPageUsesTemplate Template:Distinguish.
- HL_Tau_76 wikiPageUsesTemplate Template:Reflist.
- HL_Tau_76 wikiPageUsesTemplate Template:Starbox_astrometry.
- HL_Tau_76 wikiPageUsesTemplate Template:Starbox_begin.
- HL_Tau_76 wikiPageUsesTemplate Template:Starbox_catalog.
- HL_Tau_76 wikiPageUsesTemplate Template:Starbox_character.
- HL_Tau_76 wikiPageUsesTemplate Template:Starbox_end.
- HL_Tau_76 wikiPageUsesTemplate Template:Starbox_observe.
- HL_Tau_76 wikiPageUsesTemplate Template:Stars_of_Taurus.
- HL_Tau_76 subject Category:Objects_named_with_variable_star_designations.
- HL_Tau_76 subject Category:Pulsating_white_dwarfs.
- HL_Tau_76 subject Category:Taurus_(constellation).
- HL_Tau_76 hypernym Star.
- HL_Tau_76 type Article.
- HL_Tau_76 type CelestialBody.
- HL_Tau_76 type Place.
- HL_Tau_76 type Star.
- HL_Tau_76 type Article.
- HL_Tau_76 type Catalogue.
- HL_Tau_76 type Variable.
- HL_Tau_76 type Location.
- HL_Tau_76 type Place.
- HL_Tau_76 type Thing.
- HL_Tau_76 comment "HL Tau 76 is a variable white dwarf star of the DAV (or ZZ Ceti) type. It was observed by G. Haro and W. J. Luyten in 1961, and was the first variable white dwarf discovered when, in 1968, Arlo U. Landolt found that it varied in brightness with a period of approximately 749.5 seconds, or 12.5 minutes. Like other DAV white dwarfs, its variability arises from non-radial gravity wave pulsations within itself., § 7.".
- HL_Tau_76 label "HL Tau 76".
- HL_Tau_76 differentFrom HL_Tauri.
- HL_Tau_76 sameAs HL_Tau_76.
- HL_Tau_76 sameAs HL_Tau_76.
- HL_Tau_76 sameAs اچال_تاو_۷۶.
- HL_Tau_76 sameAs HL_Tau_76.
- HL_Tau_76 sameAs m.02y_c8c.
- HL_Tau_76 sameAs Q2349289.
- HL_Tau_76 sameAs Q2349289.
- HL_Tau_76 sameAs HL金牛座76.
- HL_Tau_76 wasDerivedFrom HL_Tau_76?oldid=632782679.
- HL_Tau_76 isPrimaryTopicOf HL_Tau_76.
- HL_Tau_76 name "HL Tau 76".