Delta Scuti variable
Subclass of pulsating star
Summary
A Delta Scuti variable is a class of pulsating star, comprising several sub-classes of object with A- or F-type spectra.
Originally created by Ketiltrout
9/13/2005, 10:17:12 PM
Modified
5/27/2026, 6:38:27 PM
Recent revisions
Add: doi-access, issue. | [[:en:WP:UCB|Use this tool]]. [[:en:WP:DBUG|Report bugs]]. | #UCB_Gadget
/* */
update table headers
/* Examples */ punctuation
clarify "old"
can be anything from main sequence to giant
"young" is a poor descriptor for stars that are typical evolving away from the main sequence - put a definition in the opening sentence, clarify details later
Removed contradictions.
Beta Cassiopeiae is not a well-known example of a Delta Scuti variable.
Dating maintenance tags: {{Needs expert}} {{Contradiction-inline}}
/* top */ tag contradiction, {{needs expert}} to resolve
Reverted 1 edit by [[Special:Contributions/205.189.94.2|205.189.94.2]] ([[User talk:205.189.94.2|talk]]) to last revision by 400Weir
More accurate colors
/* Examples */ Added some color to the table. It shouldn't be too similar because it is a somewhat wider range of stars.
/* Examples */ Added QQ Telescopii
/* Examples */ Added V701 CrA
/* Examples */
Undid revision 1147503758 by [[Special:Contributions/182.1.209.70|182.1.209.70]] ([[User talk:182.1.209.70|talk]]) poor grammar, wrong caps, merging two sentences about (slightly) different subjects
Typo
