List of stars in Canis Major

{{Short description|None}}

{{Use dmy dates|date=October 2020}}

This is the list of notable stars in the constellation Canis Major, sorted by decreasing brightness.

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List

{{Sticky header}}

class="wikitable sortable sticky-header"
Name

! B

! F

! Var

! HD

! HIP

! RA

! Dec

! vis.
mag.

! abs.
mag.

! Dist. (ly)

! Sp. class

! Notes

Sirius A, Bα94891532349{{RA|06|45|09.25}}{{DEC|−16|42|47.3}}−1.461.428.6A0m...style="text-align:left;" | Alhabor, Aschere, Canicula, the Dog Star; brightest star, 5th nearest star system; binary
ε CMaε215208933579{{RA|06|58|37.55}}{{DEC|−28|58|19.5}}1.50−4.10431B2IIstyle="text-align:left;" | Adhara, Aoul al Adzari, Prima Virginum[http://articles.adsabs.harvard.edu//full/1895MNRAS..55..429K/0000432.000.html E.B Knobel – On a catalogue of stars in the Calendarium of Al Achsasi Al Mouakket] part of Al ʽAdhārā or Al AdzariConsisting with ε CMa, δ CMa (Wezen), η CMa (Aludra) and ο2 CMa (Thanih al Adzari), see [https://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Canis_Major*.html Star Names, R.H. Allen, p. 130]ε CMa as Aoul al Adzari or Prima Virginum (the first virgin), ο2 CMa as Thanih al Adzari or Secunda Virginum (the second virgin) and δ CMa as Thalath al Adzari or Tertia Virginum (the third virgin). η CMa should be Rabah al Adzari or Quarta Virginum (the fourth virgin) consistently, but it was given by the name Aludra, meaning the virgin (same meaning with Adhara (ε CMa) or Al ʽAdhārā)
δ CMaδ255460534444{{RA|07|08|23.49}}{{DEC|−26|23|35.5}}1.83−6.871791F8Iastyle="text-align:left;" | Wezen, Thalath al Adzari, Tertia Virginum, part of Al ʽAdhārā or Al Adzari; variable star, {{VSA|0.004|24.08478}}
β CMaβ24474330324{{RA|06|22|41.99}}{{DEC|−17|57|21.3}}1.98−3.95499B1II/IIIstyle="text-align:left;" | Mirzam (Murzim); β Cep variable, {{Variable star|1.93|2|0.25003}}
η CMaη315835035904{{RA|07|24|05.71}}{{DEC|−29|18|11.2}}2.45−7.513196B5Iastyle="text-align:left;" | Aludra, part of Al ʽAdhārā or Al Adzari; α Cyg variable
ζ CMaζ14440230122{{RA|06|20|18.79}}{{DEC|−30|03|48.2}}3.02−2.05336B2.5Vstyle="text-align:left;" | Furud; spectroscopic binary; suspected variable
ο2 CMaο2245313833977{{RA|07|03|01.47}}{{DEC|−23|49|59.9}}3.02−6.462567B3Iastyle="text-align:left;" |Thanih al Adzari, Secunda Virginum, part of Al ʽAdhārā or Al Adzari; α Cyg variable
σ CMaσ225287733856{{RA|07|01|43.15}}{{DEC|−27|56|05.4}}3.49−4.371216K4IIIstyle="text-align:left;"|Unurgunite, irregular variable, {{Variable star|3.43|3.51}}
κ CMaκ135001332759{{RA|06|49|50.47}}{{DEC|−32|30|30.6}}3.50−3.42789B1.5IVnestyle="text-align:left;" | γ Cas variable, {{Variable star|3.40|3.97}}
ο1 CMaο1165087733152{{RA|06|54|07.95}}{{DEC|−24|11|03.2}}3.89−5.021976K3Iabstyle="text-align:left;" | irregular variable, {{Variable star|3.78|3.99}}
ν2 CMaν274720531592{{RA|06|36|41.00}}{{DEC|−19|15|20.6}}3.952.4665K1III+...style="text-align:left;" |Yějī (野雞),{{in lang|zh}} [http://aeea.nmns.edu.tw/2006/0607/ap060716.html AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 16 日] has a planet (b); suspected variable, {{Variable star|3.87|3.96}}
ω CMaω285613935037{{RA|07|14|48.66}}{{DEC|−26|46|21.7}}4.01−3.25924B2IV/Vestyle="text-align:left;" | γ Cas variable, {{Variable star|3.54|4.18}}
θ CMaθ145077833160{{RA|06|54|11.48}}{{DEC|−12|02|18.9}}4.08−0.36252K4III
γ CMaγ235324434045{{RA|07|03|45.49}}{{DEC|−15|37|59.7}}4.12−1.34402B8IIstyle="text-align:left;" | Muliphein; suspected variable
ξ1 CMaξ144632831125{{RA|06|31|51.37}}{{DEC|−23|25|06.4}}4.34−4.652050B1IIIstyle="text-align:left;" | β Cep variable, {{Variable star|4.33|4.36|0.2095755}}
ι CMaι205130933347{{RA|06|56|08.23}}{{DEC|−17|03|15.3}}4.36−5.513075B3Ib/IIstyle="text-align:left;" | β Cep variable, {{Variable star|4.36|4.4|0.08}}
τ CMaτ305706135415{{RA|07|18|42.49}}{{DEC|−24|57|15.8}}4.37−5.593196O9Ibstyle="text-align:left;" | member of the NGC 2362 star cluster; β Lyr variable
ν3 CMaν384744231700{{RA|06|37|53.43}}{{DEC|−18|14|14.8}}4.42−1.35464K0II/III
27 CMa27EW5601434981{{RA|07|14|15.22}}{{DEC|−26|21|09.1}}4.42−4.001575B3IIIestyle="text-align:left;" | binary, component A spectroscopic binary, component B γ Cas variable, {{Variable star|4.42|4.82}}
λ CMaλ4581330788{{RA|06|28|10.22}}{{DEC|−32|34|48.5}}4.47−1.01406B4V
ξ2 CMaξ254693331416{{RA|06|35|03.38}}{{DEC|−22|57|53.4}}4.54−0.97412A0III
π CMaπ195119933302{{RA|06|55|37.40}}{{DEC|−20|08|11.7}}4.662.3395F2IV/Vvariable star, {{VSA|0.002|0.09013}}
HD 566185661835205{{RA|07|16|35.00}}{{DEC|−27|52|52.6}}4.66−1.05453M2IIIsuspected variable
HD 476674766731827{{RA|06|39|16.72}}{{DEC|−14|08|44.7}}4.82−3.601575K2III
15 CMa15EY5070733092{{RA|06|53|32.91}}{{DEC|−20|13|27.3}}4.82−3.651614B1IVstyle="text-align:left;" | β Cep variable, {{Variable star|4.79|4.84|0.184557}}
145 G. CMaThis star is Gould's 145th of Canis Major in his Uranometria Argentina. (Gould, B. A., (2009) Uranometria Argentina, (Reprinted and updated by Pilcher, F.)[http://www.uranometriaargentina.com/] {{Webarchive|url=https://web.archive.org/web/20120227032716/http://www.uranometriaargentina.com/ |date=27 February 2012 }}) Kostjuk (see abovew) erroneously lists it as simply "145 CMa". SIMBAD follows this error in its object query result as " [http://simbad.u-strasbg.fr/simbad/sim-id?Ident=145%20CMa * 145 CMa – Star]".5657735210{{RA|07|16|36.84}}{{DEC|−23|18|56.2}}4.83−6.596269K4IIIDouble star; suspected variable, {{Variable star|4.78|4.86}}
UW CMa29UW5706035412{{RA|07|18|40.38}}{{DEC|−24|33|31.3}}4.88−4.932991O7Ia:fpstyle="text-align:left;" | β Lyr variable, {{Variable star|4.84|5.33|4.393407}}
HD 578215782135727{{RA|07|22|13.53}}{{DEC|−19|00|59.7}}4.94−1.06517B5II/III
HD 434454344529735{{RA|06|15|44.88}}{{DEC|−13|43|06.2}}5.00−0.30375B9V
μ CMaμ185125033345{{RA|06|56|06.65}}{{DEC|−14|02|36.4}}5.00−2.22908B9.5Vstyle="text-align:left;" | Isis
HD 438274382729895{{RA|06|17|41.73}}{{DEC|−16|48|57.3}}5.15−1.05567K1III
HD 461844618431084{{RA|06|31|23.02}}{{DEC|−12|23|30.9}}5.160.05343K1III
HD 58343FW5834335951{{RA|07|24|40.19}}{{DEC|−16|12|05.1}}5.18−2.13945B2Vnestyle="text-align:left;" | γ Cas variable, {{Variable star|5.|5.5}}
HD 449514495130457{{RA|06|24|10.35}}{{DEC|−11|31|48.0}}5.21−0.34420K3III
10 CMa10FT4891732292{{RA|06|44|28.47}}{{DEC|−31|04|13.9}}5.23−4.292608B2Vstyle="text-align:left;" | γ Cas variable, {{Variable star|5.13|5.44}}
HD 475364753631688{{RA|06|37|47.54}}{{DEC|−32|20|23.6}}5.25−0.17396K1IIIstyle="text-align:left;" | has two planets (b & c)
11 CMa114922932492{{RA|06|46|51.09}}{{DEC|−14|25|33.6}}5.28−1.19642B8/B9III
HD 512835128333316{{RA|06|55|46.93}}{{DEC|−22|56|29.2}}5.28−3.822159B2/B3IIIsuspected variable
HD 571465714635427{{RA|07|18|51.28}}{{DEC|−26|35|09.1}}5.29−2.801353G2IIsuspected variable
HD 490484904832411{{RA|06|45|59.40}}{{DEC|−14|47|45.9}}5.30−0.13398A1IV/V
HD 585355853535957{{RA|07|24|43.87}}{{DEC|−31|48|32.1}}5.35−0.79552K1IIIsuspected variable, {{Variable star|5.31|5.43}}
HD 563425634235083{{RA|07|15|21.08}}{{DEC|−30|41|11.3}}5.36−1.12646B2Vsuspected variable, {{VSA|0.006}}
HD 582155821535848{{RA|07|23|28.97}}{{DEC|−27|50|03.4}}5.37−0.76549K4IIIvariable star, {{VSA|0.008|20.67397}}
HD 496624966232677{{RA|06|48|57.74}}{{DEC|−15|08|41.0}}5.39−0.96607B7IVvariable star, {{VSA|0.010|1.43019}}
NO CMaNO5815535795{{RA|07|23|00.70}}{{DEC|−31|55|25.6}}5.40−2.811430B3Vstyle="text-align:left;" | Be star
FN CMaFN5397434301{{RA|07|06|40.77}}{{DEC|−11|17|38.5}}5.41−4.292835B0.5IVstyle="text-align:left;" | β Cep variable, {{Variable star|5.38|5.42|0.08866}}
HD 582865828635855{{RA|07|23|31.90}}{{DEC|−32|12|07.5}}5.41−2.341156B2/B3II/III
HD 517335173333478{{RA|06|57|33.97}}{{DEC|−24|37|51.8}}5.452.52126F3V
HD 550705507034624{{RA|07|10|19.33}}{{DEC|−27|29|29.5}}5.46−1.01643G8III
HD 564055640535180{{RA|07|16|14.58}}{{DEC|−15|35|08.4}}5.460.82277A1Vsuspected variable
FR CMaFR4445830214{{RA|06|21|24.72}}{{DEC|−11|46|23.7}}5.48−3.071672B1Vpe SBstyle="text-align:left;" | γ Cas variable, {{Variable star|5.46|5.64}}
HD 439554395529941{{RA|06|18|13.73}}{{DEC|−19|58|01.2}}5.51−1.91994B2/B3V
HD 561605616035044{{RA|07|14|51.19}}{{DEC|−27|02|16.5}}5.580.97273K3IIIvariable star, {{VSA|0.006|4.45653}}
HD 520185201833575{{RA|06|58|35.90}}{{DEC|−25|24|51.0}}5.59−1.931042B2V
HD 574785747835615{{RA|07|20|58.29}}{{DEC|−14|21|37.8}}5.59−0.57556G8/K0III
NR CMaNR5895436186{{RA|07|27|07.99}}{{DEC|−17|51|53.5}}5.600.93280F2Vstyle="text-align:left;" |δ Sct variable
HD 450184501830436{{RA|06|23|55.91}}{{DEC|−25|34|39.1}}5.61−1.04697K5IIIsuspected variable
HD 469364693631362{{RA|06|34|35.33}}{{DEC|−32|42|58.5}}5.62−0.25487B9V
HR 2501HP4913132385{{RA|06|45|31.19}}{{DEC|−30|56|56.4}}5.62−2.811583B+...style="text-align:left;" | γ Cas and λ Eri variable, {{Variable star|5.33|5.81|0.79187}}
LS CMaLS5267033804{{RA|07|01|05.95}}{{DEC|−25|12|56.3}}5.64−1.851028B2/B3III/IVeclipsing binary
HD 506445064433077{{RA|06|53|18.84}}{{DEC|−19|01|58.0}}5.650.63329A9/F0III
FY CMaFY5897836168{{RA|07|26|59.49}}{{DEC|−23|05|09.7}}5.65−2.541417B1IIγ Cas variable, {{Variable star|4.8|6.25}}
LZ CMaLZ5491234579{{RA|07|09|43.03}}{{DEC|−25|13|51.8}}5.69−3.061831B2Vstyle="text-align:left;" | β Lyr variable, {{VSA|0.03}}
HD 479464794631870{{RA|06|39|42.67}}{{DEC|−30|28|12.1}}5.701.36241K1III
R CMaR5716735487{{RA|07|19|28.08}}{{DEC|−16|23|41.7}}5.702.48144F2III/IVstyle="text-align:left;" | Algol variable, {{Variable star|5.7|6.34|1.1359405}}
ν1 CMaν164713831564{{RA|06|36|22.86}}{{DEC|−18|39|35.8}}5.711.07277G8III/F3V...
HD 465474654731190{{RA|06|32|38.98}}{{DEC|−32|01|49.6}}5.73−1.32838B2Vsuspected variable, {{VSA|5.64|5.72}}
IY CMaIY4587130840{{RA|06|28|39.24}}{{DEC|−32|22|16.7}}5.74−1.27823B5IVstyle="text-align:left;" | Be star; eclipsing binary
HD 50123HZ5012332810{{RA|06|50|23.35}}{{DEC|−31|42|21.9}}5.74−0.97718B3Vrotating ellipsoidal variable, {{Variable star|5.71|5.79}}
FV CMaFV5430934360{{RA|07|07|22.59}}{{DEC|−23|50|26.6}}5.75−4.042964B2V:nnstyle="text-align:left;" | γ Cas variable, {{Variable star|5.64|5.94}}
HD 457654576530836{{RA|06|28|37.41}}{{DEC|−17|27|57.7}}5.760.19424K0III
HD 499804998032809{{RA|06|50|21.77}}{{DEC|−17|05|04.4}}5.77−2.621552K3III
HD 555895558934888{{RA|07|13|07.20}}{{DEC|−11|15|04.9}}5.77−0.77661K0
HD 440814408130011{{RA|06|18|58.98}}{{DEC|−20|55|32.2}}5.79−2.971842B3II/IIIsuspected β Cep variable
HD 584615846135998{{RA|07|25|08.44}}{{DEC|−13|45|07.1}}5.793.08114F3V
HD 586125861236024{{RA|07|25|25.27}}{{DEC|−25|13|04.0}}5.79−4.193228B5III
HD 590675906736251{{RA|07|27|51.66}}{{DEC|−11|33|24.7}}5.79−1.661009B8Vv comp VBγ Cas variable, {{Variable star|5.73|5.90}}
17 CMa175105533248{{RA|06|55|02.74}}{{DEC|−20|24|17.5}}5.80−0.54605A2V
HD 553445534434758{{RA|07|11|41.61}}{{DEC|−20|52|59.2}}5.84−0.04489A0IV/V
MZ CMaMZ5761535626{{RA|07|21|04.34}}{{DEC|−25|53|30.0}}5.87−0.86723M3IIIsemiregular variable
HD 433964339629679{{RA|06|15|08.40}}{{DEC|−20|16|20.1}}5.88−1.39929K2IIIvariable star, {{VSA|0.008|2.42919}}
26 CMa26MM5552234798{{RA|07|12|12.22}}{{DEC|−25|56|33.4}}5.91−0.80718B2IV/Vstyle="text-align:left;" | 53 Per variable
HD 461894618931037{{RA|06|30|46.29}}{{DEC|−27|46|10.5}}5.92−1.781128B3IV/Vvariable star, {{VSA|0.005|3.28106}}
HD 490954909532366{{RA|06|45|23.08}}{{DEC|−31|47|34.5}}5.923.9979F7V
HD 471824718231599{{RA|06|36|46.60}}{{DEC|−13|19|15.5}}5.95−0.91769K4/K5III
HD 557625576234914{{RA|07|13|24.01}}{{DEC|−22|40|26.9}}5.96−0.90780K4IIIsuspected variable, {{VSA|0.14}}
HD 435444354429771{{RA|06|16|07.70}}{{DEC|−16|37|04.8}}5.97−1.07836B2/B3Vsuspected variable, {{Variable star|5.71|5.97}}
HD 434294342929692{{RA|06|15|17.71}}{{DEC|−18|28|37.2}}5.991.96208K1III
OS CMaOS5476434561{{RA|07|09|33.37}}{{DEC|−16|14|04.2}}6.00B1Ib/IIstyle="text-align:left;" | α Cyg variable
HR 2800HQ5759335611{{RA|07|20|54.92}}{{DEC|−26|57|49.9}}6.00−2.711801B3Vstyle="text-align:left;" | Algol variable, {{Variable star|5.99|6.25|24.6033}}
HD 475614756131758{{RA|06|38|35.43}}{{DEC|−16|52|24.6}}6.010.26460A0IV
HD 565785657835213{{RA|07|16|38.38}}{{DEC|−23|18|39.8}}6.021.53258A5m...
HD 440214402129993{{RA|06|18|48.79}}{{DEC|−15|01|30.0}}6.04−0.73738M1III:suspected variable, {{Variable star|5.96|6.06}}
HD 490014900132368{{RA|06|45|23.38}}{{DEC|−23|27|45.0}}6.040.15492K2III
HD 585855858536017{{RA|07|25|19.98}}{{DEC|−21|58|57.4}}6.04−3.903165A6II
HD 437454374529843{{RA|06|17|03.52}}{{DEC|−22|42|52.6}}6.053.04130F8/G0V
HD 455884558830711{{RA|06|27|11.48}}{{DEC|−25|51|21.5}}6.053.6797F8/G0V
HD 478274782731859{{RA|06|39|36.22}}{{DEC|−23|41|44.3}}6.05−0.32614A0V
HD 508065080633094{{RA|06|53|33.76}}{{DEC|−28|32|19.4}}6.053.9984G3/G5V
HD 571185711835442{{RA|07|19|01.92}}{{DEC|−19|16|49.1}}6.11F2Iasuspected variable, {{Variable star|6.08|6.11}}
12 CMa12HK4933332504{{RA|06|47|01.49}}{{DEC|−21|00|55.5}}6.07−0.49668B7II/IIIstyle="text-align:left;" | α2 CVn variable
HD 536295362934142{{RA|07|04|47.04}}{{DEC|−22|01|53.8}}6.091.07330K2IIICN...
HD 541735417334318{{RA|07|06|52.48}}{{DEC|−24|57|38.1}}6.09−1.28970K2IIIvariable star, {{VSA|0.005|17.08526}}
HD 555685556834782{{RA|07|12|04.12}}{{DEC|−30|49|17.1}}6.102.71155A8III/IV
HD 473664736631674{{RA|06|37|40.79}}{{DEC|−12|59|05.3}}6.111.46277K1III:has two planets (b & c)
HD 449964499630468{{RA|06|24|20.58}}{{DEC|−12|57|43.0}}6.12−2.731918B4Vsuspected variable
GY CMaGY5585734924{{RA|07|13|36.45}}{{DEC|−27|21|22.9}}6.12−4.885175B2IIstyle="text-align:left;" | β Cep variable, {{VSA|0.04|0.112}}
HD 506435064333079{{RA|06|53|21.85}}{{DEC|−18|55|58.5}}6.130.39458A3III
HD 460644606431024{{RA|06|30|34.89}}{{DEC|−13|08|53.4}}6.16−1.571148B2IIIsuspected variable
HD 583465834635920{{RA|07|24|17.24}}{{DEC|−22|54|46.0}}6.20−0.31652B8/B9V
HD 518235182333492{{RA|06|57|42.64}}{{DEC|−27|32|15.1}}6.22−1.251019B2/B3Vsuspected variable
HD 508535085333126{{RA|06|53|55.46}}{{DEC|−24|32|19.5}}6.230.43472A0V
HD 549585495834617{{RA|07|10|09.36}}{{DEC|−18|41|08.1}}6.232.74162F3V
HD 584395843935975{{RA|07|24|50.88}}{{DEC|−19|00|44.2}}6.24−2.451781A2Ib/IIsuspected variable
HD 48501V3504850132144{{RA|06|42|46.08}}{{DEC|−22|26|55.8}}6.262.81159F2Vstyle="text-align:left;" | γ Dor variable, {{Variable star|6.18|6.27|0.91401}}
HD 522735227333666{{RA|06|59|39.26}}{{DEC|−21|36|10.4}}6.26−1.901399B2III
HD 448914489130420{{RA|06|23|46.14}}{{DEC|−15|04|16.5}}6.27−2.151575K2/K3III
HD 526195261933760{{RA|07|00|42.53}}{{DEC|−28|29|22.1}}6.282.11222F3/F5V
HD 442254422530062{{RA|06|19|38.19}}{{DEC|−22|06|11.3}}6.29−0.61784K3IIIsuspected variable
HD 46407HR4640731205{{RA|06|32|46.88}}{{DEC|−11|09|59.0}}6.300.88395K0III:...style="text-align:left;" | Algol variable, {{Variable star|6.24|6.32}}
HD 567315673135241{{RA|07|16|57.22}}{{DEC|−30|53|49.0}}6.300.46481A9II
HD 449564495630376{{RA|06|23|14.50}}{{DEC|−31|47|25.1}}6.311.27332G8III
KM CMaKM4634731086{{RA|06|31|24.01}}{{DEC|−32|52|06.8}}6.31−1.10988M4IIIsemiregular variable
HD 498914989132744{{RA|06|49|44.00}}{{DEC|−24|04|33.7}}6.310.04584A0/A1V
HD 443944439430190{{RA|06|21|05.43}}{{DEC|−11|49|02.4}}6.32−1.701309K5
HD 454204542030669{{RA|06|26|42.66}}{{DEC|−14|36|12.2}}6.320.14560K0/K1III
HD 470124701231469{{RA|06|35|30.81}}{{DEC|−22|06|32.4}}6.320.33513K0III
HD 500935009332827{{RA|06|50|36.96}}{{DEC|−25|46|42.3}}6.32−1.521203B2III/IV
HD 523485234833703{{RA|07|00|08.29}}{{DEC|−20|09|30.4}}6.32−1.501194B3V
HD 559855598534954{{RA|07|13|57.34}}{{DEC|−30|20|23.3}}6.32−1.921449B2IIIsuspected variable
HD 587665876636045{{RA|07|25|42.99}}{{DEC|−31|44|19.4}}6.32−1.09988B2/B3IIIsuspected variable
KX CMaKX5064833040{{RA|06|53|00.31}}{{DEC|−26|57|26.9}}6.33−0.70830M6IIIsemiregular variable
HR 2680IL5403134248{{RA|07|06|00.49}}{{DEC|−30|39|20.6}}6.34−0.69830B3VAlgol and 53 Per variable, {{Variable star|6.32|6.54|8.09858}}
HD 558565585634940{{RA|07|13|48.39}}{{DEC|−22|54|20.8}}6.34−2.081575B2IVsuspected variable
HD 563415634135132{{RA|07|15|47.30}}{{DEC|−23|44|25.1}}6.34−0.89911A0V
V415 CMaV4154724731593{{RA|06|36|41.07}}{{DEC|−22|36|53.1}}6.35−0.46751B3VAlgol variable, {{Variable star|6.34|6.48|1.98571}}
HD 514115141133330{{RA|06|55|54.78}}{{DEC|−31|47|24.7}}6.36−1.831417B3VBe star, {{VSA|0.015}}
HD 519255192533532{{RA|06|58|07.56}}{{DEC|−27|09|51.8}}6.36−1.891455B2Vsuspected variable
V352 CMaV3524316229568{{RA|06|13|45.33}}{{DEC|−23|51|43.9}}6.375.2654G5VBY Dra variable, {{Variable star|6.35|6.40|7.2}}
HD 451844518430503{{RA|06|24|43.99}}{{DEC|−28|46|47.3}}6.374.6572G2Vhas a planet (b)
HD 466024660231266{{RA|06|33|26.68}}{{DEC|−20|55|26.0}}6.391.12368K0III+...
HD 521405214033591{{RA|06|58|43.70}}{{DEC|−30|59|53.0}}6.41−0.46771B3V
HD 489384893832322{{RA|06|44|51.96}}{{DEC|−27|20|32.6}}6.434.3187F7V
HD 460374603730988{{RA|06|30|11.81}}{{DEC|−19|12|53.4}}6.44−1.491259M0/M1IIIsuspected variable
HD 568765687635326{{RA|07|17|48.01}}{{DEC|−26|47|51.2}}6.45−0.80921B5Vn
HD 475794757931736{{RA|06|38|22.91}}{{DEC|−23|34|49.1}}6.48−0.07667A2V
HD 539755397534297{{RA|07|06|35.97}}{{DEC|−12|23|38.2}}6.48−4.424939B7Iab...
HD 443794437930141{{RA|06|20|35.17}}{{DEC|−23|38|16.1}}6.490.03639K0III
HD 42927IP4292729488{{RA|06|12|46.33}}{{DEC|−17|45|47.6}}6.49908B5II/IIIrotating ellipsoidal variable, {{Variable star|6.50|6.54|5.0946}}
FU CMaFU5243733721{{RA|07|00|19.36}}{{DEC|−22|07|08.6}}6.512100B3Vnnγ Cas variable, {{Variable star|6.48|6.6}}
W CMaW5436134413{{RA|07|08|03.44}}{{DEC|−11|55|23.8}}6.568400Csemiregular variable, {{Variable star|6.27|7.09|160}}
GU CMaGU5272133868{{RA|07|01|49.51}}{{DEC|−11|18|03.3}}6.591450B2Vneβ Lyr variable, {{Variable star|6.49|6.72|1.610137}}
HR 2724HN5559534814{{RA|07|12|24.18}}{{DEC|−27|28|29.1}}6.61805A5IV-Vδ Sct variable, {{VSA|0.025}}
EZ CMaEZ5089633165{{RA|06|54|13.04}}{{DEC|−23|55|42.0}}6.914500WN4-sWolf–Rayet star, {{Variable star|6.71|6.95|3.763}}
HD 471864718631540{{RA|06|36|08.79}}{{DEC|−27|37|20.3}}7.84.9123G6Vstyle=text-align:left; | has two planets (b & c)
VY CMaVY5806135793{{RA|07|22|58.29}}{{DEC|−25|46|03.5}}7.95−9.43900M2.5–M5e Iastyle="text-align:left;" | One of the largest known stars; semiregular variable or irregular variable, {{Variable star|6.5|9.6}}
GZ CMaGZ5642935187{{RA|07|16|09.21}}{{DEC|−16|43|00.1}}7.971290A0III/IVAlgol variable, {{Variable star|7.97|8.51|4.80085}}
HD 453644536430579{{RA|06|25|38.48}}{{DEC|−31|28|51.4}}8.075.50106G8Vstyle="text-align:left;" | has two planets (b & c)
FZ CMaFZ5294233953{{RA|07|02|42.61}}{{DEC|−11|27|11.6}}8.141350B2IVnAlgol variable, {{Variable star|8.05|8.44|1.27306}}
HD 45677FS4567730800{{RA|06|28|17.42}}{{DEC|−13|03|11.1}}8.50908Bpsheprototype FS CMa variable, {{Variable star|7.35|8.58}}
Z CMaZ5317934042{{RA|07|03|43.16}}{{DEC|−11|33|06.2}}8.802630BpeEXor and FU Ori variable, {{Variable star|8.2|10.6}}
HD 431974319729550{{RA|06|13|35.66}}{{DEC|−29|53|50.2}}8.955.25179G9IV-Vstyle="text-align:left;" | Amadioha,{{Cite web|url=http://www.nameexoworlds.iau.org/final-results|title=Approved names|website=NameExoWorlds|language=en|access-date=2020-01-02}}{{Cite web|url=https://www.iau.org/news/pressreleases/detail/iau1912/|title=International Astronomical Union {{!}} IAU|website=www.iau.org|access-date=2020-01-02}} has a planet (b)
SW CMaSW5452034431{{RA|07|08|15.24}}{{DEC|−22|26|25.3}}9.162230A3IVAlgol variable, {{Variable star|9.15|9.68|10.091988}}
WASP-101{{RA|06|33|24.0}}{{DEC
23|29|10}}10.3F6style="text-align:left;" | has a transiting planet (b)
HD 569255692535378{{RA|07|18|29.13}}{{DEC|−13|13|01.5}}11.403700WN4-sWolf–Rayet star at center of NGC 2359
DZ CMaDZ{{RA|07|16|59.33}}{{DEC|−15|18|25.4}}11.6G0double-mode Cepheid variable, {{Variable star|11.6|12.4|2.311}}
HATS-4{{RA|06|16|27.0}}{{DEC
21|27|11}}13.51370style="text-align:left;" | has a planet (b)
EUVE J0720-317IN{{RA|07|20|47.91}}{{DEC|−31|47|02.7}}14.64DA.9re-radiating binary system, {{Variable star|14.64|14.89|1.262396}}
RX J0720.4-3125{{RA|07|20|24.96}}{{DEC|−31|25|50.2}}26.61174one of the nearest neutron stars
PSR B0628-28{{RA|06|30|49.48}}{{DEC|−28|34|43.1}}pulsar
CX CMa{{RA|07|22|00.9896}}{{DEC|−25|52|35.912}}9.66000-7000B5Veclipsing binary, {{Variable star|9.9|10.6|0.954625}}
NN CMaNN5801135769{{RA|07|22|43.32}}{{DEC
26|00|40.9}}7.19-12.853397B1/B2Ib/IIn{{Starlist Legend}}

See also

References

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  • {{ cite web

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| access-date = 13 December 2017 }}

{{reflist}}

{{Lists of stars by constellation}}

{{Stars of Canis Major}}

*List

Canis Major