Matches in DBpedia 2014 for { <http://dbpedia.org/resource/Instability_strip> ?p ?o. }
Showing items 1 to 36 of
36
with 100 items per page.
- Instability_strip abstract "The instability strip is a nearly vertical region in the Hertzsprung–Russell diagram which is occupied by pulsating variable stars: RR Lyrae variables where it intersects the horizontal branch; classical Cepheid variables where it crosses the supergiants; W Virginis variables at slightly lower luminosities; and Delta Scuti variables near the main sequence, including SX Phoenicis variables and rapidly oscillating Ap (roAp) stars.RV Tauri variables are also often considered to lie on the instability strip near the Cepheids. Although they are a very different type of star, their pulsations have been shown to be due to the same basic mechanism.".
- Instability_strip thumbnail HR-diag-instability-strip.svg?width=300.
- Instability_strip wikiPageID "5571489".
- Instability_strip wikiPageRevisionID "592223165".
- Instability_strip hasPhotoCollection Instability_strip.
- Instability_strip subject Category:Hertzsprung–Russell_classifications.
- Instability_strip subject Category:Stellar_evolution.
- Instability_strip type Abstraction100002137.
- Instability_strip type Act100030358.
- Instability_strip type Activity100407535.
- Instability_strip type Categorization101012712.
- Instability_strip type Event100029378.
- Instability_strip type Grouping101012360.
- Instability_strip type Hertzsprung-RussellClassifications.
- Instability_strip type PsychologicalFeature100023100.
- Instability_strip type YagoPermanentlyLocatedEntity.
- Instability_strip comment "The instability strip is a nearly vertical region in the Hertzsprung–Russell diagram which is occupied by pulsating variable stars: RR Lyrae variables where it intersects the horizontal branch; classical Cepheid variables where it crosses the supergiants; W Virginis variables at slightly lower luminosities; and Delta Scuti variables near the main sequence, including SX Phoenicis variables and rapidly oscillating Ap (roAp) stars.RV Tauri variables are also often considered to lie on the instability strip near the Cepheids. ".
- Instability_strip label "Bande d'instabilité".
- Instability_strip label "Instability strip".
- Instability_strip label "Instabilitätsstreifen".
- Instability_strip label "Striscia di instabilità".
- Instability_strip label "Полоса нестабильности".
- Instability_strip label "不安定帯".
- Instability_strip label "不穩定帶".
- Instability_strip sameAs Instabilitätsstreifen.
- Instability_strip sameAs Bande_d'instabilité.
- Instability_strip sameAs Striscia_di_instabilità.
- Instability_strip sameAs 不安定帯.
- Instability_strip sameAs 불안정띠.
- Instability_strip sameAs m.0dt35t.
- Instability_strip sameAs Q280157.
- Instability_strip sameAs Q280157.
- Instability_strip sameAs Instability_strip.
- Instability_strip wasDerivedFrom Instability_strip?oldid=592223165.
- Instability_strip depiction HR-diag-instability-strip.svg.
- Instability_strip isPrimaryTopicOf Instability_strip.
