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- Q830831 subject Q5894358.
- Q830831 subject Q7217185.
- Q830831 subject Q8728797.
- Q830831 subject Q9311209.
- Q830831 abstract "Beta Lyrae variables are a class of close binary stars. Their total brightness is variable because the two component stars orbit each other, and in this orbit one component periodically passes in front of the other one, thereby blocking its light. The two component stars of Beta Lyrae systems are quite heavy (several solar masses (M☉) each) and extended (giants or supergiants). They are so close, that their shapes are heavily distorted by mutual gravitation forces: the stars have ellipsoidal shapes, and there are extensive mass flows from one component to the other.".
- Q830831 wikiPageExternalLink vartype.txt.
- Q830831 wikiPageExternalLink gcvs.
- Q830831 wikiPageWikiLink Q10264906.
- Q830831 wikiPageWikiLink Q11412.
- Q830831 wikiPageWikiLink Q1202327.
- Q830831 wikiPageWikiLink Q124313.
- Q830831 wikiPageWikiLink Q13352.
- Q830831 wikiPageWikiLink Q141022.
- Q830831 wikiPageWikiLink Q15510436.
- Q830831 wikiPageWikiLink Q159190.
- Q830831 wikiPageWikiLink Q179600.
- Q830831 wikiPageWikiLink Q180892.
- Q830831 wikiPageWikiLink Q193599.
- Q830831 wikiPageWikiLink Q232086.
- Q830831 wikiPageWikiLink Q2398989.
- Q830831 wikiPageWikiLink Q24452.
- Q830831 wikiPageWikiLink Q253525.
- Q830831 wikiPageWikiLink Q2538697.
- Q830831 wikiPageWikiLink Q2660595.
- Q830831 wikiPageWikiLink Q2717822.
- Q830831 wikiPageWikiLink Q375172.
- Q830831 wikiPageWikiLink Q3781521.
- Q830831 wikiPageWikiLink Q50053.
- Q830831 wikiPageWikiLink Q5177456.
- Q830831 wikiPageWikiLink Q531.
- Q830831 wikiPageWikiLink Q5875.
- Q830831 wikiPageWikiLink Q5894358.
- Q830831 wikiPageWikiLink Q603757.
- Q830831 wikiPageWikiLink Q6243.
- Q830831 wikiPageWikiLink Q6472.
- Q830831 wikiPageWikiLink Q654396.
- Q830831 wikiPageWikiLink Q675076.
- Q830831 wikiPageWikiLink Q691269.
- Q830831 wikiPageWikiLink Q7217185.
- Q830831 wikiPageWikiLink Q775489.
- Q830831 wikiPageWikiLink Q8728797.
- Q830831 wikiPageWikiLink Q9311209.
- Q830831 comment "Beta Lyrae variables are a class of close binary stars. Their total brightness is variable because the two component stars orbit each other, and in this orbit one component periodically passes in front of the other one, thereby blocking its light. The two component stars of Beta Lyrae systems are quite heavy (several solar masses (M☉) each) and extended (giants or supergiants).".
- Q830831 label "Beta Lyrae variable".