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==References== {{reflist|refs= <ref name=Csizmadia2004>{{cite journal | title=On the properties of contact binary stars | last1=Csizmadia | first1=Sz. | last2=Klagyivik | first2=P. | journal=Astronomy and Astrophysics | volume=426 | pages=1001β1005 | date=November 2004 | issue=3 | arxiv=astro-ph/0408049 | bibcode=2004A&A...426.1001C | doi=10.1051/0004-6361:20040430 }}</ref> <ref name=DarlingBinary>{{Cite web | url=http://www.daviddarling.info/encyclopedia/B/binarystar.html | title=binary star | last=Darling | first=David | website=www.daviddarling.info | access-date=2019-05-06 }}</ref> <ref name=Thompson2006>{{cite book | title=An Introduction to Astrophysical Fluid Dynamics | first=Michael J. | last=Thompson | publication-place=London | publisher=Imperial College Press | pages=51β53 | year=2006 | isbn=1-86094-615-1 }}</ref> <ref name=Tassoul2000>{{cite book | title=Stellar Rotation | page=231 | first1=Jean Louis | last1=Tassoul | first2=Andrew | last2=King | first3=Douglas | last3=Lin | first4=Stephen P. | last4=Maran | first5=Jim | last5=Pringle | first6=Martin | last6=Ward | display-authors=1 | publication-place=Cambridge, UK, New York | publisher=Cambridge University Press | year=2000 | isbn=0-521-77218-4 }}</ref> <ref name=Mullaney2005>{{cite book | title=Double and Multiple Stars and how to Observe Them | first=James | last=Mullaney | publication-place=New York, London | publisher=Springer | page=19 | year=2005 | isbn=1-85233-751-6 }}</ref> <ref name=Ivanova2013>{{cite journal | last1=Ivanova | first1=N. | last2=Justham | first2=S. | last3=Chen | first3=X. | last4=De Marco | first4=O. | last5=Fryer | first5=C. L. | last6=Gaburov | first6=E. | last7=Ge | first7=H. | last8=Glebbeek | first8=E. | last9=Han | first9=Z. | last10=Li | first10=X. D. | last11=Lu | first11=G. | last12=Podsiadlowski | first12=P. | last13=Potter | first13=A. | last14=Soker | first14=N. | last15=Taam | first15=R. | last16=Tauris | first16=T. M. | last17=van den Heuvel | first17=E. P. J. | last18=Webbink | first18=R. F. | title=Common envelope evolution: where we stand and how we can move forward | display-authors=1 | journal=The Astronomy and Astrophysics Review | year=2013 | volume=21 | pages=59 | bibcode=2013A&ARv..21...59I | arxiv=1209.4302 | doi=10.1007/s00159-013-0059-2 }}</ref> <ref name=Kuiper1941>{{cite journal | url=http://articles.adsabs.harvard.edu/pdf/1941ApJ....93..133K | last1=Kuiper | first1=Gerard P. | title=On the Interpretation of Ξ² Lyrae and Other Close Binaries | journal=Astrophysical Journal | year=1941 | volume=93 | pages=133 | bibcode=1941ApJ....93..133K | doi=10.1086/144252 |doi-access=free}}</ref> }} [[Category:Binary stars|*]]
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