Zeta Aurigae: Difference between revisions

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''ζ Aurigae'' ([[Latinisation of names|Latinised]] to ''Zeta Aurigae'') is the system's [[Bayer designation]]. The designations of the two components as ''ζ Aurigae A'' and ''B'' derive from the convention used by the Washington Multiplicity Catalog (WMC) for [[Star system|multiple star system]]s, and adopted by the [[International Astronomical Union]] (IAU).<ref name="planetnaming"/>
 
The system bore the traditional names ''Haedus I'' (also ''Hoedus'') and ''Sadatoni'' (rarely ''Saclateni'').<ref name=Rumrill/> It was one of the two ''haedi'' ([[Latin]]: 'kids') of the she-goat [[Capella]], the other being Haedus II, [[Eta Aurigae]]. The name Sadatoni is from the [[Arabic]] الساعد الثاني ''as-sā<sup>c</sup>id aθ-θānī'' "the second arm (of the charioteer)". The rare traditional name ''Azaleh'' is shared (in the form ''Hassaleh'') with [[Iota Aurigae]].<ref name=kaler/> In 2016, the IAU organized a [[IAU Working Group on Star Names|Working Group on Star Names]] (WGSN)<ref name="WGSN"/> to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire [[multiple star|multiple systems]].<ref name="TriRpt18"/> It approved the names ''Saclateni'' for the component Zeta Aurigae A and ''Haedus'' for [[Eta Aurigae]] on 30 June 2017 and they are both now so included in the List of IAU-approved Star Names.<ref name="IAU-LSN"/>
 
In [[Chinese astronomy|Chinese]], {{lang|zh|柱}} ({{lang|zh-Latn|Zhù}}), meaning ''[[Net (Chinese constellation)|Pillars]]'', refers to an [[Asterism (astronomy)|asterism]] consisting of Zeta Aurigae, [[Epsilon Aurigae]], Eta Aurigae, [[Upsilon Aurigae]], [[Nu Aurigae]], [[Tau Aurigae]], [[Chi Aurigae]] and [[26 Aurigae]].<ref name=zh/> Consequently, the [[Chinese star names|Chinese name]] for Zeta Aurigae itself is {{lang|zh|柱二}} ({{lang|zh-Latn|Zhù èr}}, {{lang-langx|en|the Second Star of Pillars}}.)<ref name=lcsd/>
 
== Properties ==
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| last3=Brown | first3=Alexander | last4=Hummel | first4=Christian A.
| title=The Masses and Radii of the Eclipsing Binary zeta Aurigae
| journal=Astrophysical Journal | date=November 1996 | volume=471 | issue=1 | page=454
| bibcode=1996ApJ...471..454B | doi=10.1086/177981 | doi-access=free }}</ref>
 
<ref name=harper2016>{{Cite journal |lastlast1=Harper |firstfirst1=G. M. |last2=Griffin |first2=R. E. M. |last3=Bennett |first3=P. D. |last4=O'Riain |first4=N. |date=2016-02-01 |title=Orbitally modulated photoexcited Si I emission in the eclipsing composite-spectrum binary ζ Aurigae |bibcode=2016MNRAS.456.1346H |journal=Monthly Notices of the Royal Astronomical Society |volume=456 |issue=2 |pages=1346–1358 |doi=10.1093/mnras/stv2668 |doi-access=free |issn=0035-8711}}</ref>
 
<ref name=Anderson2012>{{citation
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<ref name=paspj19_209>{{citation | last1=Kiyokawa | first1=M. | title=Photoelectric Observation of Zeta Aurigae during the 1963-64 Eclipse | journal=Publications of the Astronomical Society of Japan | volume=19 | page=209 | date=1967 | bibcode=1967PASJ...19..209K | postscript=. }}</ref>
 
<ref name=an331_4_349>{{citation | last1=Hohle | first1=M. M. | last2=Neuhäuser | first2=R. | last3=Schutz | first3=B. F. | title=Masses and luminosities of O- and B-type stars and red supergiants | journal=Astronomische Nachrichten | volume=331 | issue=4 | page=349 |date=April 2010 | doi=10.1002/asna.200911355 | bibcode=2010AN....331..349H | arxiv=1003.2335 | s2cid=111387483 | postscript=. }}</ref>
 
<ref name=apj679_2_1490>{{citation | last1=Eaton | first1=Joel A. | last2=Henry | first2=Gregory W. | last3=Odell | first3=Andrew P. | title=Orbits and Pulsations of the Classical ζ Aurigae Binaries | journal=The Astrophysical Journal | volume=679 | issue=2 | pages=1490–1498 |date=June 2008 | doi=10.1086/587452 | bibcode=2008ApJ...679.1490E | postscript=. |arxiv = 0802.2238 | s2cid=2079219 }}</ref>
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[[Category:Bright Star Catalogue objects|1612]]
[[Category:Stars with proper names|Sadatoni]]
[[Category:K-type supergiants]]