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
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Name
! B ! F ! Var ! HD ! HIP ! RA ! Dec ! vis. ! abs. ! Notes | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
Sirius A, B | α | 9 | 48915 | 32349 | {{RA|06|45|09.25}} | {{DEC|−16|42|47.3}} | −1.46 | 1.42 | 8.6 | A0m... | style="text-align:left;" | Alhabor, Aschere, Canicula, the Dog Star; brightest star, 5th nearest star system; binary | |
ε CMa | ε | 21 | 52089 | 33579 | {{RA|06|58|37.55}} | {{DEC|−28|58|19.5}} | 1.50 | −4.10 | 431 | B2II | style="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 CMa | δ | 25 | 54605 | 34444 | {{RA|07|08|23.49}} | {{DEC|−26|23|35.5}} | 1.83 | −6.87 | 1791 | F8Ia | style="text-align:left;" | Wezen, Thalath al Adzari, Tertia Virginum, part of Al ʽAdhārā or Al Adzari; variable star, {{VSA|0.004|24.08478}} | |
β CMa | β | 2 | 44743 | 30324 | {{RA|06|22|41.99}} | {{DEC|−17|57|21.3}} | 1.98 | −3.95 | 499 | B1II/III | style="text-align:left;" | Mirzam (Murzim); β Cep variable, {{Variable star|1.93|2|0.25003}} | |
η CMa | η | 31 | 58350 | 35904 | {{RA|07|24|05.71}} | {{DEC|−29|18|11.2}} | 2.45 | −7.51 | 3196 | B5Ia | style="text-align:left;" | Aludra, part of Al ʽAdhārā or Al Adzari; α Cyg variable | |
ζ CMa | ζ | 1 | 44402 | 30122 | {{RA|06|20|18.79}} | {{DEC|−30|03|48.2}} | 3.02 | −2.05 | 336 | B2.5V | style="text-align:left;" | Furud; spectroscopic binary; suspected variable | |
ο2 CMa | ο2 | 24 | 53138 | 33977 | {{RA|07|03|01.47}} | {{DEC|−23|49|59.9}} | 3.02 | −6.46 | 2567 | B3Ia | style="text-align:left;" |Thanih al Adzari, Secunda Virginum, part of Al ʽAdhārā or Al Adzari; α Cyg variable | |
σ CMa | σ | 22 | 52877 | 33856 | {{RA|07|01|43.15}} | {{DEC|−27|56|05.4}} | 3.49 | −4.37 | 1216 | K4III | style="text-align:left;"|Unurgunite, irregular variable, {{Variable star|3.43|3.51}} | |
κ CMa | κ | 13 | 50013 | 32759 | {{RA|06|49|50.47}} | {{DEC|−32|30|30.6}} | 3.50 | −3.42 | 789 | B1.5IVne | style="text-align:left;" | γ Cas variable, {{Variable star|3.40|3.97}} | |
ο1 CMa | ο1 | 16 | 50877 | 33152 | {{RA|06|54|07.95}} | {{DEC|−24|11|03.2}} | 3.89 | −5.02 | 1976 | K3Iab | style="text-align:left;" | irregular variable, {{Variable star|3.78|3.99}} | |
ν2 CMa | ν2 | 7 | 47205 | 31592 | {{RA|06|36|41.00}} | {{DEC|−19|15|20.6}} | 3.95 | 2.46 | 65 | K1III+... | 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 CMa | ω | 28 | 56139 | 35037 | {{RA|07|14|48.66}} | {{DEC|−26|46|21.7}} | 4.01 | −3.25 | 924 | B2IV/Ve | style="text-align:left;" | γ Cas variable, {{Variable star|3.54|4.18}} | |
θ CMa | θ | 14 | 50778 | 33160 | {{RA|06|54|11.48}} | {{DEC|−12|02|18.9}} | 4.08 | −0.36 | 252 | K4III | ||
γ CMa | γ | 23 | 53244 | 34045 | {{RA|07|03|45.49}} | {{DEC|−15|37|59.7}} | 4.12 | −1.34 | 402 | B8II | style="text-align:left;" | Muliphein; suspected variable | |
ξ1 CMa | ξ1 | 4 | 46328 | 31125 | {{RA|06|31|51.37}} | {{DEC|−23|25|06.4}} | 4.34 | −4.65 | 2050 | B1III | style="text-align:left;" | β Cep variable, {{Variable star|4.33|4.36|0.2095755}} | |
ι CMa | ι | 20 | 51309 | 33347 | {{RA|06|56|08.23}} | {{DEC|−17|03|15.3}} | 4.36 | −5.51 | 3075 | B3Ib/II | style="text-align:left;" | β Cep variable, {{Variable star|4.36|4.4|0.08}} | |
τ CMa | τ | 30 | 57061 | 35415 | {{RA|07|18|42.49}} | {{DEC|−24|57|15.8}} | 4.37 | −5.59 | 3196 | O9Ib | style="text-align:left;" | member of the NGC 2362 star cluster; β Lyr variable | |
ν3 CMa | ν3 | 8 | 47442 | 31700 | {{RA|06|37|53.43}} | {{DEC|−18|14|14.8}} | 4.42 | −1.35 | 464 | K0II/III | ||
27 CMa | 27 | EW | 56014 | 34981 | {{RA|07|14|15.22}} | {{DEC|−26|21|09.1}} | 4.42 | −4.00 | 1575 | B3IIIe | style="text-align:left;" | binary, component A spectroscopic binary, component B γ Cas variable, {{Variable star|4.42|4.82}} | |
λ CMa | λ | 45813 | 30788 | {{RA|06|28|10.22}} | {{DEC|−32|34|48.5}} | 4.47 | −1.01 | 406 | B4V | |||
ξ2 CMa | ξ2 | 5 | 46933 | 31416 | {{RA|06|35|03.38}} | {{DEC|−22|57|53.4}} | 4.54 | −0.97 | 412 | A0III | ||
π CMa | π | 19 | 51199 | 33302 | {{RA|06|55|37.40}} | {{DEC|−20|08|11.7}} | 4.66 | 2.33 | 95 | F2IV/V | variable star, {{VSA|0.002|0.09013}} | |
HD 56618 | 56618 | 35205 | {{RA|07|16|35.00}} | {{DEC|−27|52|52.6}} | 4.66 | −1.05 | 453 | M2III | suspected variable | |||
HD 47667 | 47667 | 31827 | {{RA|06|39|16.72}} | {{DEC|−14|08|44.7}} | 4.82 | −3.60 | 1575 | K2III | ||||
15 CMa | 15 | EY | 50707 | 33092 | {{RA|06|53|32.91}} | {{DEC|−20|13|27.3}} | 4.82 | −3.65 | 1614 | B1IV | style="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]". | 56577 | 35210 | {{RA|07|16|36.84}} | {{DEC|−23|18|56.2}} | 4.83 | −6.59 | 6269 | K4III | Double star; suspected variable, {{Variable star|4.78|4.86}} | |||
UW CMa | 29 | UW | 57060 | 35412 | {{RA|07|18|40.38}} | {{DEC|−24|33|31.3}} | 4.88 | −4.93 | 2991 | O7Ia:fp | style="text-align:left;" | β Lyr variable, {{Variable star|4.84|5.33|4.393407}} | |
HD 57821 | 57821 | 35727 | {{RA|07|22|13.53}} | {{DEC|−19|00|59.7}} | 4.94 | −1.06 | 517 | B5II/III | ||||
HD 43445 | 43445 | 29735 | {{RA|06|15|44.88}} | {{DEC|−13|43|06.2}} | 5.00 | −0.30 | 375 | B9V | ||||
μ CMa | μ | 18 | 51250 | 33345 | {{RA|06|56|06.65}} | {{DEC|−14|02|36.4}} | 5.00 | −2.22 | 908 | B9.5V | style="text-align:left;" | Isis | |
HD 43827 | 43827 | 29895 | {{RA|06|17|41.73}} | {{DEC|−16|48|57.3}} | 5.15 | −1.05 | 567 | K1III | ||||
HD 46184 | 46184 | 31084 | {{RA|06|31|23.02}} | {{DEC|−12|23|30.9}} | 5.16 | 0.05 | 343 | K1III | ||||
HD 58343 | FW | 58343 | 35951 | {{RA|07|24|40.19}} | {{DEC|−16|12|05.1}} | 5.18 | −2.13 | 945 | B2Vne | style="text-align:left;" | γ Cas variable, {{Variable star|5.|5.5}} | ||
HD 44951 | 44951 | 30457 | {{RA|06|24|10.35}} | {{DEC|−11|31|48.0}} | 5.21 | −0.34 | 420 | K3III | ||||
10 CMa | 10 | FT | 48917 | 32292 | {{RA|06|44|28.47}} | {{DEC|−31|04|13.9}} | 5.23 | −4.29 | 2608 | B2V | style="text-align:left;" | γ Cas variable, {{Variable star|5.13|5.44}} | |
HD 47536 | 47536 | 31688 | {{RA|06|37|47.54}} | {{DEC|−32|20|23.6}} | 5.25 | −0.17 | 396 | K1III | style="text-align:left;" | has two planets (b & c) | |||
11 CMa | 11 | 49229 | 32492 | {{RA|06|46|51.09}} | {{DEC|−14|25|33.6}} | 5.28 | −1.19 | 642 | B8/B9III | |||
HD 51283 | 51283 | 33316 | {{RA|06|55|46.93}} | {{DEC|−22|56|29.2}} | 5.28 | −3.82 | 2159 | B2/B3III | suspected variable | |||
HD 57146 | 57146 | 35427 | {{RA|07|18|51.28}} | {{DEC|−26|35|09.1}} | 5.29 | −2.80 | 1353 | G2II | suspected variable | |||
HD 49048 | 49048 | 32411 | {{RA|06|45|59.40}} | {{DEC|−14|47|45.9}} | 5.30 | −0.13 | 398 | A1IV/V | ||||
HD 58535 | 58535 | 35957 | {{RA|07|24|43.87}} | {{DEC|−31|48|32.1}} | 5.35 | −0.79 | 552 | K1III | suspected variable, {{Variable star|5.31|5.43}} | |||
HD 56342 | 56342 | 35083 | {{RA|07|15|21.08}} | {{DEC|−30|41|11.3}} | 5.36 | −1.12 | 646 | B2V | suspected variable, {{VSA|0.006}} | |||
HD 58215 | 58215 | 35848 | {{RA|07|23|28.97}} | {{DEC|−27|50|03.4}} | 5.37 | −0.76 | 549 | K4III | variable star, {{VSA|0.008|20.67397}} | |||
HD 49662 | 49662 | 32677 | {{RA|06|48|57.74}} | {{DEC|−15|08|41.0}} | 5.39 | −0.96 | 607 | B7IV | variable star, {{VSA|0.010|1.43019}} | |||
NO CMa | NO | 58155 | 35795 | {{RA|07|23|00.70}} | {{DEC|−31|55|25.6}} | 5.40 | −2.81 | 1430 | B3V | style="text-align:left;" | Be star | ||
FN CMa | FN | 53974 | 34301 | {{RA|07|06|40.77}} | {{DEC|−11|17|38.5}} | 5.41 | −4.29 | 2835 | B0.5IV | style="text-align:left;" | β Cep variable, {{Variable star|5.38|5.42|0.08866}} | ||
HD 58286 | 58286 | 35855 | {{RA|07|23|31.90}} | {{DEC|−32|12|07.5}} | 5.41 | −2.34 | 1156 | B2/B3II/III | ||||
HD 51733 | 51733 | 33478 | {{RA|06|57|33.97}} | {{DEC|−24|37|51.8}} | 5.45 | 2.52 | 126 | F3V | ||||
HD 55070 | 55070 | 34624 | {{RA|07|10|19.33}} | {{DEC|−27|29|29.5}} | 5.46 | −1.01 | 643 | G8III | ||||
HD 56405 | 56405 | 35180 | {{RA|07|16|14.58}} | {{DEC|−15|35|08.4}} | 5.46 | 0.82 | 277 | A1V | suspected variable | |||
FR CMa | FR | 44458 | 30214 | {{RA|06|21|24.72}} | {{DEC|−11|46|23.7}} | 5.48 | −3.07 | 1672 | B1Vpe SB | style="text-align:left;" | γ Cas variable, {{Variable star|5.46|5.64}} | ||
HD 43955 | 43955 | 29941 | {{RA|06|18|13.73}} | {{DEC|−19|58|01.2}} | 5.51 | −1.91 | 994 | B2/B3V | ||||
HD 56160 | 56160 | 35044 | {{RA|07|14|51.19}} | {{DEC|−27|02|16.5}} | 5.58 | 0.97 | 273 | K3III | variable star, {{VSA|0.006|4.45653}} | |||
HD 52018 | 52018 | 33575 | {{RA|06|58|35.90}} | {{DEC|−25|24|51.0}} | 5.59 | −1.93 | 1042 | B2V | ||||
HD 57478 | 57478 | 35615 | {{RA|07|20|58.29}} | {{DEC|−14|21|37.8}} | 5.59 | −0.57 | 556 | G8/K0III | ||||
NR CMa | NR | 58954 | 36186 | {{RA|07|27|07.99}} | {{DEC|−17|51|53.5}} | 5.60 | 0.93 | 280 | F2V | style="text-align:left;" |δ Sct variable | ||
HD 45018 | 45018 | 30436 | {{RA|06|23|55.91}} | {{DEC|−25|34|39.1}} | 5.61 | −1.04 | 697 | K5III | suspected variable | |||
HD 46936 | 46936 | 31362 | {{RA|06|34|35.33}} | {{DEC|−32|42|58.5}} | 5.62 | −0.25 | 487 | B9V | ||||
HR 2501 | HP | 49131 | 32385 | {{RA|06|45|31.19}} | {{DEC|−30|56|56.4}} | 5.62 | −2.81 | 1583 | B+... | style="text-align:left;" | γ Cas and λ Eri variable, {{Variable star|5.33|5.81|0.79187}} | ||
LS CMa | LS | 52670 | 33804 | {{RA|07|01|05.95}} | {{DEC|−25|12|56.3}} | 5.64 | −1.85 | 1028 | B2/B3III/IV | eclipsing binary | ||
HD 50644 | 50644 | 33077 | {{RA|06|53|18.84}} | {{DEC|−19|01|58.0}} | 5.65 | 0.63 | 329 | A9/F0III | ||||
FY CMa | FY | 58978 | 36168 | {{RA|07|26|59.49}} | {{DEC|−23|05|09.7}} | 5.65 | −2.54 | 1417 | B1II | γ Cas variable, {{Variable star|4.8|6.25}} | ||
LZ CMa | LZ | 54912 | 34579 | {{RA|07|09|43.03}} | {{DEC|−25|13|51.8}} | 5.69 | −3.06 | 1831 | B2V | style="text-align:left;" | β Lyr variable, {{VSA|0.03}} | ||
HD 47946 | 47946 | 31870 | {{RA|06|39|42.67}} | {{DEC|−30|28|12.1}} | 5.70 | 1.36 | 241 | K1III | ||||
R CMa | R | 57167 | 35487 | {{RA|07|19|28.08}} | {{DEC|−16|23|41.7}} | 5.70 | 2.48 | 144 | F2III/IV | style="text-align:left;" | Algol variable, {{Variable star|5.7|6.34|1.1359405}} | ||
ν1 CMa | ν1 | 6 | 47138 | 31564 | {{RA|06|36|22.86}} | {{DEC|−18|39|35.8}} | 5.71 | 1.07 | 277 | G8III/F3V... | ||
HD 46547 | 46547 | 31190 | {{RA|06|32|38.98}} | {{DEC|−32|01|49.6}} | 5.73 | −1.32 | 838 | B2V | suspected variable, {{VSA|5.64|5.72}} | |||
IY CMa | IY | 45871 | 30840 | {{RA|06|28|39.24}} | {{DEC|−32|22|16.7}} | 5.74 | −1.27 | 823 | B5IV | style="text-align:left;" | Be star; eclipsing binary | ||
HD 50123 | HZ | 50123 | 32810 | {{RA|06|50|23.35}} | {{DEC|−31|42|21.9}} | 5.74 | −0.97 | 718 | B3V | rotating ellipsoidal variable, {{Variable star|5.71|5.79}} | ||
FV CMa | FV | 54309 | 34360 | {{RA|07|07|22.59}} | {{DEC|−23|50|26.6}} | 5.75 | −4.04 | 2964 | B2V:nn | style="text-align:left;" | γ Cas variable, {{Variable star|5.64|5.94}} | ||
HD 45765 | 45765 | 30836 | {{RA|06|28|37.41}} | {{DEC|−17|27|57.7}} | 5.76 | 0.19 | 424 | K0III | ||||
HD 49980 | 49980 | 32809 | {{RA|06|50|21.77}} | {{DEC|−17|05|04.4}} | 5.77 | −2.62 | 1552 | K3III | ||||
HD 55589 | 55589 | 34888 | {{RA|07|13|07.20}} | {{DEC|−11|15|04.9}} | 5.77 | −0.77 | 661 | K0 | ||||
HD 44081 | 44081 | 30011 | {{RA|06|18|58.98}} | {{DEC|−20|55|32.2}} | 5.79 | −2.97 | 1842 | B3II/III | suspected β Cep variable | |||
HD 58461 | 58461 | 35998 | {{RA|07|25|08.44}} | {{DEC|−13|45|07.1}} | 5.79 | 3.08 | 114 | F3V | ||||
HD 58612 | 58612 | 36024 | {{RA|07|25|25.27}} | {{DEC|−25|13|04.0}} | 5.79 | −4.19 | 3228 | B5III | ||||
HD 59067 | 59067 | 36251 | {{RA|07|27|51.66}} | {{DEC|−11|33|24.7}} | 5.79 | −1.66 | 1009 | B8Vv comp VB | γ Cas variable, {{Variable star|5.73|5.90}} | |||
17 CMa | 17 | 51055 | 33248 | {{RA|06|55|02.74}} | {{DEC|−20|24|17.5}} | 5.80 | −0.54 | 605 | A2V | |||
HD 55344 | 55344 | 34758 | {{RA|07|11|41.61}} | {{DEC|−20|52|59.2}} | 5.84 | −0.04 | 489 | A0IV/V | ||||
MZ CMa | MZ | 57615 | 35626 | {{RA|07|21|04.34}} | {{DEC|−25|53|30.0}} | 5.87 | −0.86 | 723 | M3III | semiregular variable | ||
HD 43396 | 43396 | 29679 | {{RA|06|15|08.40}} | {{DEC|−20|16|20.1}} | 5.88 | −1.39 | 929 | K2III | variable star, {{VSA|0.008|2.42919}} | |||
26 CMa | 26 | MM | 55522 | 34798 | {{RA|07|12|12.22}} | {{DEC|−25|56|33.4}} | 5.91 | −0.80 | 718 | B2IV/V | style="text-align:left;" | 53 Per variable | |
HD 46189 | 46189 | 31037 | {{RA|06|30|46.29}} | {{DEC|−27|46|10.5}} | 5.92 | −1.78 | 1128 | B3IV/V | variable star, {{VSA|0.005|3.28106}} | |||
HD 49095 | 49095 | 32366 | {{RA|06|45|23.08}} | {{DEC|−31|47|34.5}} | 5.92 | 3.99 | 79 | F7V | ||||
HD 47182 | 47182 | 31599 | {{RA|06|36|46.60}} | {{DEC|−13|19|15.5}} | 5.95 | −0.91 | 769 | K4/K5III | ||||
HD 55762 | 55762 | 34914 | {{RA|07|13|24.01}} | {{DEC|−22|40|26.9}} | 5.96 | −0.90 | 780 | K4III | suspected variable, {{VSA|0.14}} | |||
HD 43544 | 43544 | 29771 | {{RA|06|16|07.70}} | {{DEC|−16|37|04.8}} | 5.97 | −1.07 | 836 | B2/B3V | suspected variable, {{Variable star|5.71|5.97}} | |||
HD 43429 | 43429 | 29692 | {{RA|06|15|17.71}} | {{DEC|−18|28|37.2}} | 5.99 | 1.96 | 208 | K1III | ||||
OS CMa | OS | 54764 | 34561 | {{RA|07|09|33.37}} | {{DEC|−16|14|04.2}} | 6.00 | B1Ib/II | style="text-align:left;" | α Cyg variable | ||||
HR 2800 | HQ | 57593 | 35611 | {{RA|07|20|54.92}} | {{DEC|−26|57|49.9}} | 6.00 | −2.71 | 1801 | B3V | style="text-align:left;" | Algol variable, {{Variable star|5.99|6.25|24.6033}} | ||
HD 47561 | 47561 | 31758 | {{RA|06|38|35.43}} | {{DEC|−16|52|24.6}} | 6.01 | 0.26 | 460 | A0IV | ||||
HD 56578 | 56578 | 35213 | {{RA|07|16|38.38}} | {{DEC|−23|18|39.8}} | 6.02 | 1.53 | 258 | A5m... | ||||
HD 44021 | 44021 | 29993 | {{RA|06|18|48.79}} | {{DEC|−15|01|30.0}} | 6.04 | −0.73 | 738 | M1III: | suspected variable, {{Variable star|5.96|6.06}} | |||
HD 49001 | 49001 | 32368 | {{RA|06|45|23.38}} | {{DEC|−23|27|45.0}} | 6.04 | 0.15 | 492 | K2III | ||||
HD 58585 | 58585 | 36017 | {{RA|07|25|19.98}} | {{DEC|−21|58|57.4}} | 6.04 | −3.90 | 3165 | A6II | ||||
HD 43745 | 43745 | 29843 | {{RA|06|17|03.52}} | {{DEC|−22|42|52.6}} | 6.05 | 3.04 | 130 | F8/G0V | ||||
HD 45588 | 45588 | 30711 | {{RA|06|27|11.48}} | {{DEC|−25|51|21.5}} | 6.05 | 3.67 | 97 | F8/G0V | ||||
HD 47827 | 47827 | 31859 | {{RA|06|39|36.22}} | {{DEC|−23|41|44.3}} | 6.05 | −0.32 | 614 | A0V | ||||
HD 50806 | 50806 | 33094 | {{RA|06|53|33.76}} | {{DEC|−28|32|19.4}} | 6.05 | 3.99 | 84 | G3/G5V | ||||
HD 57118 | 57118 | 35442 | {{RA|07|19|01.92}} | {{DEC|−19|16|49.1}} | 6.11 | F2Ia | suspected variable, {{Variable star|6.08|6.11}} | |||||
12 CMa | 12 | HK | 49333 | 32504 | {{RA|06|47|01.49}} | {{DEC|−21|00|55.5}} | 6.07 | −0.49 | 668 | B7II/III | style="text-align:left;" | α2 CVn variable | |
HD 53629 | 53629 | 34142 | {{RA|07|04|47.04}} | {{DEC|−22|01|53.8}} | 6.09 | 1.07 | 330 | K2IIICN... | ||||
HD 54173 | 54173 | 34318 | {{RA|07|06|52.48}} | {{DEC|−24|57|38.1}} | 6.09 | −1.28 | 970 | K2III | variable star, {{VSA|0.005|17.08526}} | |||
HD 55568 | 55568 | 34782 | {{RA|07|12|04.12}} | {{DEC|−30|49|17.1}} | 6.10 | 2.71 | 155 | A8III/IV | ||||
HD 47366 | 47366 | 31674 | {{RA|06|37|40.79}} | {{DEC|−12|59|05.3}} | 6.11 | 1.46 | 277 | K1III: | has two planets (b & c) | |||
HD 44996 | 44996 | 30468 | {{RA|06|24|20.58}} | {{DEC|−12|57|43.0}} | 6.12 | −2.73 | 1918 | B4V | suspected variable | |||
GY CMa | GY | 55857 | 34924 | {{RA|07|13|36.45}} | {{DEC|−27|21|22.9}} | 6.12 | −4.88 | 5175 | B2II | style="text-align:left;" | β Cep variable, {{VSA|0.04|0.112}} | ||
HD 50643 | 50643 | 33079 | {{RA|06|53|21.85}} | {{DEC|−18|55|58.5}} | 6.13 | 0.39 | 458 | A3III | ||||
HD 46064 | 46064 | 31024 | {{RA|06|30|34.89}} | {{DEC|−13|08|53.4}} | 6.16 | −1.57 | 1148 | B2III | suspected variable | |||
HD 58346 | 58346 | 35920 | {{RA|07|24|17.24}} | {{DEC|−22|54|46.0}} | 6.20 | −0.31 | 652 | B8/B9V | ||||
HD 51823 | 51823 | 33492 | {{RA|06|57|42.64}} | {{DEC|−27|32|15.1}} | 6.22 | −1.25 | 1019 | B2/B3V | suspected variable | |||
HD 50853 | 50853 | 33126 | {{RA|06|53|55.46}} | {{DEC|−24|32|19.5}} | 6.23 | 0.43 | 472 | A0V | ||||
HD 54958 | 54958 | 34617 | {{RA|07|10|09.36}} | {{DEC|−18|41|08.1}} | 6.23 | 2.74 | 162 | F3V | ||||
HD 58439 | 58439 | 35975 | {{RA|07|24|50.88}} | {{DEC|−19|00|44.2}} | 6.24 | −2.45 | 1781 | A2Ib/II | suspected variable | |||
HD 48501 | V350 | 48501 | 32144 | {{RA|06|42|46.08}} | {{DEC|−22|26|55.8}} | 6.26 | 2.81 | 159 | F2V | style="text-align:left;" | γ Dor variable, {{Variable star|6.18|6.27|0.91401}} | ||
HD 52273 | 52273 | 33666 | {{RA|06|59|39.26}} | {{DEC|−21|36|10.4}} | 6.26 | −1.90 | 1399 | B2III | ||||
HD 44891 | 44891 | 30420 | {{RA|06|23|46.14}} | {{DEC|−15|04|16.5}} | 6.27 | −2.15 | 1575 | K2/K3III | ||||
HD 52619 | 52619 | 33760 | {{RA|07|00|42.53}} | {{DEC|−28|29|22.1}} | 6.28 | 2.11 | 222 | F3/F5V | ||||
HD 44225 | 44225 | 30062 | {{RA|06|19|38.19}} | {{DEC|−22|06|11.3}} | 6.29 | −0.61 | 784 | K3III | suspected variable | |||
HD 46407 | HR | 46407 | 31205 | {{RA|06|32|46.88}} | {{DEC|−11|09|59.0}} | 6.30 | 0.88 | 395 | K0III:... | style="text-align:left;" | Algol variable, {{Variable star|6.24|6.32}} | ||
HD 56731 | 56731 | 35241 | {{RA|07|16|57.22}} | {{DEC|−30|53|49.0}} | 6.30 | 0.46 | 481 | A9II | ||||
HD 44956 | 44956 | 30376 | {{RA|06|23|14.50}} | {{DEC|−31|47|25.1}} | 6.31 | 1.27 | 332 | G8III | ||||
KM CMa | KM | 46347 | 31086 | {{RA|06|31|24.01}} | {{DEC|−32|52|06.8}} | 6.31 | −1.10 | 988 | M4III | semiregular variable | ||
HD 49891 | 49891 | 32744 | {{RA|06|49|44.00}} | {{DEC|−24|04|33.7}} | 6.31 | 0.04 | 584 | A0/A1V | ||||
HD 44394 | 44394 | 30190 | {{RA|06|21|05.43}} | {{DEC|−11|49|02.4}} | 6.32 | −1.70 | 1309 | K5 | ||||
HD 45420 | 45420 | 30669 | {{RA|06|26|42.66}} | {{DEC|−14|36|12.2}} | 6.32 | 0.14 | 560 | K0/K1III | ||||
HD 47012 | 47012 | 31469 | {{RA|06|35|30.81}} | {{DEC|−22|06|32.4}} | 6.32 | 0.33 | 513 | K0III | ||||
HD 50093 | 50093 | 32827 | {{RA|06|50|36.96}} | {{DEC|−25|46|42.3}} | 6.32 | −1.52 | 1203 | B2III/IV | ||||
HD 52348 | 52348 | 33703 | {{RA|07|00|08.29}} | {{DEC|−20|09|30.4}} | 6.32 | −1.50 | 1194 | B3V | ||||
HD 55985 | 55985 | 34954 | {{RA|07|13|57.34}} | {{DEC|−30|20|23.3}} | 6.32 | −1.92 | 1449 | B2III | suspected variable | |||
HD 58766 | 58766 | 36045 | {{RA|07|25|42.99}} | {{DEC|−31|44|19.4}} | 6.32 | −1.09 | 988 | B2/B3III | suspected variable | |||
KX CMa | KX | 50648 | 33040 | {{RA|06|53|00.31}} | {{DEC|−26|57|26.9}} | 6.33 | −0.70 | 830 | M6III | semiregular variable | ||
HR 2680 | IL | 54031 | 34248 | {{RA|07|06|00.49}} | {{DEC|−30|39|20.6}} | 6.34 | −0.69 | 830 | B3V | Algol and 53 Per variable, {{Variable star|6.32|6.54|8.09858}} | ||
HD 55856 | 55856 | 34940 | {{RA|07|13|48.39}} | {{DEC|−22|54|20.8}} | 6.34 | −2.08 | 1575 | B2IV | suspected variable | |||
HD 56341 | 56341 | 35132 | {{RA|07|15|47.30}} | {{DEC|−23|44|25.1}} | 6.34 | −0.89 | 911 | A0V | ||||
V415 CMa | V415 | 47247 | 31593 | {{RA|06|36|41.07}} | {{DEC|−22|36|53.1}} | 6.35 | −0.46 | 751 | B3V | Algol variable, {{Variable star|6.34|6.48|1.98571}} | ||
HD 51411 | 51411 | 33330 | {{RA|06|55|54.78}} | {{DEC|−31|47|24.7}} | 6.36 | −1.83 | 1417 | B3V | Be star, {{VSA|0.015}} | |||
HD 51925 | 51925 | 33532 | {{RA|06|58|07.56}} | {{DEC|−27|09|51.8}} | 6.36 | −1.89 | 1455 | B2V | suspected variable | |||
V352 CMa | V352 | 43162 | 29568 | {{RA|06|13|45.33}} | {{DEC|−23|51|43.9}} | 6.37 | 5.26 | 54 | G5V | BY Dra variable, {{Variable star|6.35|6.40|7.2}} | ||
HD 45184 | 45184 | 30503 | {{RA|06|24|43.99}} | {{DEC|−28|46|47.3}} | 6.37 | 4.65 | 72 | G2V | has a planet (b) | |||
HD 46602 | 46602 | 31266 | {{RA|06|33|26.68}} | {{DEC|−20|55|26.0}} | 6.39 | 1.12 | 368 | K0III+... | ||||
HD 52140 | 52140 | 33591 | {{RA|06|58|43.70}} | {{DEC|−30|59|53.0}} | 6.41 | −0.46 | 771 | B3V | ||||
HD 48938 | 48938 | 32322 | {{RA|06|44|51.96}} | {{DEC|−27|20|32.6}} | 6.43 | 4.31 | 87 | F7V | ||||
HD 46037 | 46037 | 30988 | {{RA|06|30|11.81}} | {{DEC|−19|12|53.4}} | 6.44 | −1.49 | 1259 | M0/M1III | suspected variable | |||
HD 56876 | 56876 | 35326 | {{RA|07|17|48.01}} | {{DEC|−26|47|51.2}} | 6.45 | −0.80 | 921 | B5Vn | ||||
HD 47579 | 47579 | 31736 | {{RA|06|38|22.91}} | {{DEC|−23|34|49.1}} | 6.48 | −0.07 | 667 | A2V | ||||
HD 53975 | 53975 | 34297 | {{RA|07|06|35.97}} | {{DEC|−12|23|38.2}} | 6.48 | −4.42 | 4939 | B7Iab... | ||||
HD 44379 | 44379 | 30141 | {{RA|06|20|35.17}} | {{DEC|−23|38|16.1}} | 6.49 | 0.03 | 639 | K0III | ||||
HD 42927 | IP | 42927 | 29488 | {{RA|06|12|46.33}} | {{DEC|−17|45|47.6}} | 6.49 | 908 | B5II/III | rotating ellipsoidal variable, {{Variable star|6.50|6.54|5.0946}} | |||
FU CMa | FU | 52437 | 33721 | {{RA|07|00|19.36}} | {{DEC|−22|07|08.6}} | 6.51 | 2100 | B3Vnn | γ Cas variable, {{Variable star|6.48|6.6}} | |||
W CMa | W | 54361 | 34413 | {{RA|07|08|03.44}} | {{DEC|−11|55|23.8}} | 6.56 | 8400 | C | semiregular variable, {{Variable star|6.27|7.09|160}} | |||
GU CMa | GU | 52721 | 33868 | {{RA|07|01|49.51}} | {{DEC|−11|18|03.3}} | 6.59 | 1450 | B2Vne | β Lyr variable, {{Variable star|6.49|6.72|1.610137}} | |||
HR 2724 | HN | 55595 | 34814 | {{RA|07|12|24.18}} | {{DEC|−27|28|29.1}} | 6.61 | 805 | A5IV-V | δ Sct variable, {{VSA|0.025}} | |||
EZ CMa | EZ | 50896 | 33165 | {{RA|06|54|13.04}} | {{DEC|−23|55|42.0}} | 6.91 | 4500 | WN4-s | Wolf–Rayet star, {{Variable star|6.71|6.95|3.763}} | |||
HD 47186 | 47186 | 31540 | {{RA|06|36|08.79}} | {{DEC|−27|37|20.3}} | 7.8 | 4.9 | 123 | G6V | style=text-align:left; | has two planets (b & c) | |||
VY CMa | VY | 58061 | 35793 | {{RA|07|22|58.29}} | {{DEC|−25|46|03.5}} | 7.95 | −9.4 | 3900 | M2.5–M5e Ia | style="text-align:left;" | One of the largest known stars; semiregular variable or irregular variable, {{Variable star|6.5|9.6}} | ||
GZ CMa | GZ | 56429 | 35187 | {{RA|07|16|09.21}} | {{DEC|−16|43|00.1}} | 7.97 | 1290 | A0III/IV | Algol variable, {{Variable star|7.97|8.51|4.80085}} | |||
HD 45364 | 45364 | 30579 | {{RA|06|25|38.48}} | {{DEC|−31|28|51.4}} | 8.07 | 5.50 | 106 | G8V | style="text-align:left;" | has two planets (b & c) | |||
FZ CMa | FZ | 52942 | 33953 | {{RA|07|02|42.61}} | {{DEC|−11|27|11.6}} | 8.14 | 1350 | B2IVn | Algol variable, {{Variable star|8.05|8.44|1.27306}} | |||
HD 45677 | FS | 45677 | 30800 | {{RA|06|28|17.42}} | {{DEC|−13|03|11.1}} | 8.50 | 908 | Bpshe | prototype FS CMa variable, {{Variable star|7.35|8.58}} | |||
Z CMa | Z | 53179 | 34042 | {{RA|07|03|43.16}} | {{DEC|−11|33|06.2}} | 8.80 | 2630 | Bpe | EXor and FU Ori variable, {{Variable star|8.2|10.6}} | |||
HD 43197 | 43197 | 29550 | {{RA|06|13|35.66}} | {{DEC|−29|53|50.2}} | 8.95 | 5.25 | 179 | G9IV-V | style="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 CMa | SW | 54520 | 34431 | {{RA|07|08|15.24}} | {{DEC|−22|26|25.3}} | 9.16 | 2230 | A3IV | Algol variable, {{Variable star|9.15|9.68|10.091988}} | |||
WASP-101 | {{RA|06|33|24.0}} | {{DEC | ||||||||||
23|29|10}} | 10.3 | F6 | style="text-align:left;" | has a transiting planet (b) | |||||||||
HD 56925 | 56925 | 35378 | {{RA|07|18|29.13}} | {{DEC|−13|13|01.5}} | 11.40 | 3700 | WN4-s | Wolf–Rayet star at center of NGC 2359 | ||||
DZ CMa | DZ | {{RA|07|16|59.33}} | {{DEC|−15|18|25.4}} | 11.6 | G0 | double-mode Cepheid variable, {{Variable star|11.6|12.4|2.311}} | ||||||
HATS-4 | {{RA|06|16|27.0}} | {{DEC | ||||||||||
21|27|11}} | 13.5 | 1370 | style="text-align:left;" | has a planet (b) | |||||||||
EUVE J0720-317 | IN | {{RA|07|20|47.91}} | {{DEC|−31|47|02.7}} | 14.64 | DA.9 | re-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}} | 26.6 | 1174 | one 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}} | 9.6 | 6000-7000 | B5V | eclipsing binary, {{Variable star|9.9|10.6|0.954625}} | ||||||
NN CMa | NN | 58011 | 35769 | {{RA|07|22|43.32}} | {{DEC | |||||||
26|00|40.9}} | 7.19 | -12.85 | 3397 | B1/B2Ib/IIn | {{Starlist Legend}} |
See also
References
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{{reflist}}
{{Lists of stars by constellation}}
{{Stars of Canis Major}}