! style="width:25%;"|تعليق
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| [[مرزم]]
| [[Beta Canis Majoris|β CMa]]
| [[الكلب الأكبر (كوكبة)|الكلب الأكبر]]
| 1909 ([[وليام والاس كامبل]]<ref name=campbell1909>{{cite journal|last1=Campbell|first1=W. W.|title=Eleven stars having variable radial velocities.|journal=The Astrophysical Journal|volume=29|year=1909|pages=224|issn=0004-637X|doi=10.1086/141644|bibcode = 1909ApJ....29..224C }}</ref>)
| 6.031
| B1II-III
| نبضات 6.03, 6.00, و4.74 ساعة.<ref name=betacma>{{citation Citation| display-authors=1 | last1=Mazumdar | first1=A. | last2=Briquet | first2=M. | last3=Desmet | first3=M. | last4=Aerts | first4=C. | title=An asteroseismic study of the β Cephei star β Canis Majoris | journal=Astronomy and Astrophysics | volume=459 | issue=2 | pages=589–596 |date=November 2006 | doi=10.1051/0004-6361:20064980 | bibcode=2006A&A...459..589M |arxiv = astro-ph/0607261 }}</ref>
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| [[Delta Ceti|δ Cet]]
| [[قيطس (كوكبة)|قيطس]]
| <ref name="Hubrig_et_al">{{citeCite journal | display-authors=1 | last1=Hubrig | first1=S. | last2=Briquet | first2=M. | last3=De Cat | first3=P. | last4=Schoeller | first4=M. | last5=Morel | first5=T. | last6=Ilyin | first6=I. | title=New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars |date=January 2009 | bibcode=2009arXiv0901.3319H | arxiv=0901.3319 | volume=0901 | page=3319 }}</ref>
| 4<sup>m</sup>.05
| 4<sup>m</sup>.1
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| [[Alphaألفا Lupi|α Lupالسبع]]
| [[السبع (كوكبة)|السبع]]
| 1956 ([[برنارد باجيل]])<ref name=mnras116_10>{{citation Citation| last1=Pagel | first1=B. E. J. | title=Results of a search for bright β Cephei variables in the southern sky | journal=[[Monthly Notices of the Royal Astronomical Society]]| volume=116 | pages=10–24 | date=1956 | bibcode=1956MNRAS.116...10P | doi=10.1093/mnras/116.1.10 }}</ref>
| 2<sup>m</sup>.29
| 2<sup>m</sup>.34
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| [[Epsilon Lupi|ε Lup]]<ref name=aaa440_1_249>{{citation Citation| display-authors=1 | last1=Uytterhoeven | first1=K. | last2=Harmanec | first2=P. | last3=Telting | first4=J. H. | last5=Aerts | first5=C. | title=The orbit of the close spectroscopic binary epsilon Lup and the intrinsic variability of its early B-type components | journal=Astronomy and Astrophysics | volume=440 | issue=1 | pages=249–260 |date=September 2005 | doi=10.1051/0004-6361:20053009 | bibcode=2005A&A...440..249U |arxiv = astro-ph/0507376 | last4=Aerts }}</ref>
| [[السبع (كوكبة)|السبع]]
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| نظام نجوم ثلاثي؛ النجم الرئيسي [[نجم ثنائي|ثنائي طيفي]]
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| [[Iota Lupi|ι Lup]]<ref name=hipparcoscat>{{citeمرجع bookكتاب|last=ESA|date=1997|title=The HIPPARCOS and TYCHO catalogues. Astrometric and photometric star catalogues derived from the ESA HIPPARCOS Space Astrometry Mission| bibcode=1997ESASP1200.....E | isbn= 9290923997|volume=1200}}</ref>
| [[السبع (كوكبة)|السبع]]
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| [[Etaجبار Orionis|η Ori(نجم)]]
| [[الجبار (كوكبة)|الجبار]]
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