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- G_29-38 abstract "Giclas 29-38 is a variable white dwarf star of the DAV, or ZZ Ceti,whose variability is due to large-amplitude, non-radial pulsations, known as gravity waves. It was first reported to be variable by Shulov and Kopatskaya in 1974. DAV stars are like normal white dwarfs but have luminosity variations with amplitudes as high as 30%, arising from a superposition of vibrational modes with periods from 100 to 1,000 seconds. Large-amplitude DAVs generally differ from lower-amplitude DAVs by having lower temperatures, longer primary periodicities, and many peaks in their vibrational spectra with frequencies which are sums of other vibrational modes.G29-38, like other complex, large-amplitude DAV variables, has proven difficult to understand. The power spectrum or periodogram of the light curve varies over times which range from weeks to years. Usually, one strong mode dominates, although many smaller-amplitude modes are often observed. The larger-amplitude modes, however, fluctuate in and out of observability; some low-power areas show more stability. Asteroseismology uses the observed spectrum of pulsations from stars like G29-38 to infer the structure of their interiors.".
- G_29-38 thumbnail G29-38_Debris_disk.jpg?width=300.
- G_29-38 wikiPageExternalLink born_again_020207.html.
- G_29-38 wikiPageID "4099694".
- G_29-38 wikiPageRevisionID "573717282".
- G_29-38 absmagV "12.4".
- G_29-38 appmagV "13.03".
- G_29-38 bV "0.14".
- G_29-38 class "DAV4.4".
- G_29-38 constell Pisces_(constellation).
- G_29-38 epoch "J2000.0".
- G_29-38 gravity "8.15".
- G_29-38 luminosityBolometric "0.002".
- G_29-38 mass "0.7".
- G_29-38 pError "4".
- G_29-38 parallax "73.4".
- G_29-38 pmDec "-302".
- G_29-38 pmRa "-360".
- G_29-38 rI "0.2".
- G_29-38 radialV "15.3".
- G_29-38 radius "0.01".
- G_29-38 temperature "11820".
- G_29-38 uB "-0.63".
- G_29-38 vR "0".
- G_29-38 variable "DAV".
- G_29-38 subject Category:Pisces_(constellation).
- G_29-38 subject Category:Pulsating_white_dwarfs.
- G_29-38 type CelestialBody.
- G_29-38 type Star.
- G_29-38 type PhysicalBody.
- G_29-38 comment "Giclas 29-38 is a variable white dwarf star of the DAV, or ZZ Ceti,whose variability is due to large-amplitude, non-radial pulsations, known as gravity waves. It was first reported to be variable by Shulov and Kopatskaya in 1974. DAV stars are like normal white dwarfs but have luminosity variations with amplitudes as high as 30%, arising from a superposition of vibrational modes with periods from 100 to 1,000 seconds.".
- G_29-38 label "G 29-38".
- G_29-38 label "G 29-38".
- G_29-38 label "G29-38".
- G_29-38 label "G29-38".
- G_29-38 sameAs G29-38.
- G_29-38 sameAs G_29-38.
- G_29-38 sameAs G29-38.
- G_29-38 sameAs m.0bhzc1.
- G_29-38 sameAs Q1627892.
- G_29-38 sameAs Q1627892.
- G_29-38 wasDerivedFrom G_29-38?oldid=573717282.
- G_29-38 depiction G29-38_Debris_disk.jpg.
- G_29-38 isPrimaryTopicOf G_29-38.
- G_29-38 name "G29-38".