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bn:01912322n
Noun Concept
NL
No term available
EN
Stellar pulsations are caused by expansions and contractions in the outer layers as a star seeks to maintain equilibrium. Wikipedia
Relations
Sources
IS A
veranderlijke ster
HAS KIND
pulserende witte dwerg
semi-regelmatige variabele
Cepheïde
EN
slow irregular variable
Mira-veranderlijke
+17 relations
HAS INSTANCE
Rigel
Deneb
HL Tau 76
ZZ Ceti
PG 1159-035
+223 relations

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