List of stars in Crux

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

Name B Var HD HIP RA Dec vis.
mag.
abs.
mag.
Dist. (ly) Sp. class Notes
β Cruβ11112362434 12h 47m 43.32s−59° 41 19.41.25−3.92352B0.5IIIMimosa, Becrux; 20th brightest star; β Cep variable, Vmax = +1.23m, Vmin = +1.31m, P = 0.2365072 d Probable high-mass member of Lower Centaurus Crux subgroup of the Scorpius–Centaurus Association.[1]
α1 Cru (α Cru A)α110824860718 12h 26m 35.94s−63° 05 56.61.4−3.6321B0.5IVAcrux, 23rd brightest star, multiple star, spectroscopic binary. Possible member Lower Centaurus Crux subgroup of the Scorpius–Centaurus Association (debated).[1]
γ Cruγ10890361084 12h 31m 09.93s−57° 06 45.21.60−0.5688M4IIIGacrux, SRV, Vmax = +1.60m, Vmin = +1.67m
α2 Cru (α Cru B)α2108249 12h 26m 36.50s−63° 05 58.02.09−2.88321B1Vcomponent of the α Cru system. Possible member Lower Centaurus Crux subgroup of the Scorpius–Centaurus Association (debated).[1]
δ Cruδ10649059747 12h 15m 08.76s−58° 44 56.02.79−2.45364B2IVImai[2], β Cep variable; Vmax = +2.78m, Vmin = +2.80m, P = 0.151038 d
Member of the Lower Centaurus Crux subgroup of the Scorpius–Centaurus Association.[3]
ε Cruε10744660260 12h 21m 21.81s−60° 24 04.93.59−0.63228K3/K4IIIGinan, suspected variable
μ1 Cruμ111209263003 12h 54m 35.66s−57° 10 40.44.03−1.29377B2IV-Vbinary star; suspected variable; Member of the Lower Centaurus Crux subgroup of the Scorpius–Centaurus Association.[3]
ζ Cruζ10698360009 12h 18m 26.29s−64° 00 11.04.06−1.16361B2.5Vdouble star, Member of the Lower Centaurus Crux subgroup of the Scorpius–Centaurus Association.[3]
η Cruη10521159072 12h 06m 52.85s−64° 36 49.14.142.6764F2IIIdouble star
θ1 Cruθ110467158758 12h 03m 01.70s−63° 18 46.64.320.08230Amspectroscopic binary
HD 11095611095662327 12h 46m 22.75s−56° 29 19.64.62−0.80396B3Vdouble star; suspected slow irregular variable; Member of the Lower Centaurus Crux subgroup of the Scorpius–Centaurus Association.[3]
λ Cruλ11207863007 12h 54m 39.22s−59° 08 48.04.62−0.59360B4Vnβ Cep variable, ΔV = 0.02m, P = 0.3951 d, Member of the Lower Centaurus Crux subgroup of the Scorpius–Centaurus Association.[3]
ι Cruι11082962268 12h 45m 37.92s−60° 58 52.24.691.78125K1IIIoptical double
θ2 Cruθ210484158867 12h 04m 19.24s−63° 09 56.64.72−2.10753B2IVspectroscopic binary; β Cep variable, Vmax = +4.70m, Vmin = +4.74m, P = 0.0889 d
α Cru C108250 12h 26m 30.90s−63° 07 21.04.86B4IVprobable optical double with the α Cru system; suspected variable
CH CruCH11033561966 12h 41m 56.60s−59° 41 08.94.91−2.601035B6IVγ Cas variable
μ2 Cruμ211209163005 12h 54m 36.92s−57° 10 07.15.08−0.14361B5Vnecomponent of μ Cru system; γ Cas variable, Vmax = +4.99m, Vmin = +5.18m
HD 110432BZ11043262027 12h 42m 50.28s−63° 03 31.05.27−2.12982B2pehigh-mass X-ray binary; γ Cas variable, Vmax = +5.24m, Vmin = +5.45m
HD 11224411224463117 12h 55m 57.14s−56° 50 08.95.34−3.471884O9Ibemission-line star; variable star, ΔV = 0.008m, P = 2.00288 d
HD 10769610769660379 12h 22m 49.47s−57° 40 34.05.380.28342B9Vsuspected variable
BL CruBL10839660781 12h 27m 28.88s−58° 59 30.45.38−0.82566M4/M5IIIsemiregular variable, ΔV = 0.35m
HD 10396110396158379 11h 58m 15.25s−56° 19 02.35.44−1.00633B8IIIsuspected variable, Vmax = +5.43m, Vmin = +5.48m
BG CruBG10896861136 12h 31m 40.34s−59° 25 26.15.49−3.071680F5Ib-G0pCepheid variable, Vmax = +5.34m, Vmin = +5.58m, P = 3.3428 d
HD 10388410388458326 11h 57m 40.04s−62° 26 55.45.59−0.73598B3Vsuspected variable
HD 10403510403558427 11h 58m 47.67s−64° 20 22.45.59−4.112835A3Ib
DS CruDS11161362732 12h 51m 17.98s−60° 19 47.25.71−4.102991A2Iabemission-line star; α Cyg variable
HD 11190411190462894 12h 53m 21.90s−60° 19 42.65.75−4.714025B9Iasuspected variable, Vmax = +5.70m, Vmin = +6.80m
HD 10873210873260969 12h 29m 54.19s−56° 31 29.95.78−0.40562M1IIIvariable star, ΔV = 0.010m, P = 196.46365 d
HD 10606810606859517 12h 12m 21.99s−62° 57 02.85.91−4.964866B9Iasuspected variable, ΔV = 0.02m
HD 10754310754360308 12h 21m 57.44s−56° 22 27.85.91−2.731743K4III + (F)variable star, ΔV = 0.007m, P = 11.23596 d
HD 10493310493358921 12h 04m 57.25s−60° 58 05.75.95−0.59661M2IIIsuspected variable
HD 10900010900061158 12h 31m 56.15s−63° 30 21.25.961.62240A8III
κ Cruκ11197362931 12h 53m 48.92s−60° 22 34.55.98−2.551661B5Iamember of the Jewel Box star cluster (note that κ Cru usually refers to the cluster itself); variable star, ΔV = 0.014m, P = 9.53562 d
HD 11050611050662058 12h 43m 09.21s−56° 10 34.35.990.47414B9VnMember of the Lower Centaurus Crux subgroup of the Scorpius–Centaurus Association.[3]
HD 10835510835560771 12h 27m 24.85s−63° 47 20.36.02−0.50657B8IV
HD 10850110850160851 12h 28m 19.31s−64° 20 27.56.051.11317A0Vn
HD 11046111046162026 12h 42m 49.80s−55° 56 49.16.060.77372B9VMember of the Lower Centaurus Crux subgroup of the Scorpius–Centaurus Association.[3]
HD 10584110584159396 12h 11m 05.25s−61° 16 38.66.081.34290F0III
HD 10857010857060870 12h 28m 33.84s−56° 24 26.26.153.02138K0/K1III
HD 10443010443058642 12h 01m 29.26s−57° 30 13.56.161.28309A1V
DL CruDL10634359678 12h 14m 16.93s−64° 24 30.76.20−7.66~20000B1.5Iaα Cyg variable
HD 10853010853060861 12h 28m 25.71s−61° 47 41.46.210.31494K2III
HD 10543710543759200 12h 08m 24.74s−60° 50 49.76.22−2.892159K3/K4II
HD 10949210949261443 12h 35m 29.79s−61° 50 29.06.222.89151G4IV
HD 10490010490058901 12h 04m 45.29s−59° 15 11.76.301.12354B9Vn
HD 10839510839560780 12h 27m 28.84s−58° 18 59.36.35−0.79874K4III
HD 10411110411158469 11h 59m 25.62s−62° 49 51.46.36−5.859022A8II
HD 11053211053262084 12h 43m 28.40s−58° 54 09.96.41−0.14667K0/K1IIIdouble star
γ Cru Bγ108925 12h 31m 16.70s−57° 04 52.06.42A3Vcomponent of the γ Cru system
T CruT10744760259 12h 21m 21.13s−62° 16 53.96.584000G2IbCepheid variable, Vmax = +6.32m, Vmin = +6.83m, P = 6.73331 d
S CruS11204462986 12h 54m 22.00s−58° 25 50.26.582300F7Ib-IICepheid variable, Vmax = +6.22m, Vmin = +6.92m, P = 4.68997 d
R CruR10780560455 12h 23m 37.69s−61° 37 44.96.900.94508F7Ib/IICepheid variable, Vmax = +6.40m, Vmin = +7.23m, P = 5.82575 d
HD 10814710814760644 12h 25m 46.27s−64° 01 19.56.994.05126F9VTupã; has a planet (b)
AG CruAG110258 12h 41m 25.98s−59° 47 38.87.90F8Ib-IICepheid variable, Vmax = +7.73m, Vmin = +8.58m, P = 3.83728 d
HD 10690610690659960 12h 17m 53.19s−55° 58 31.897.8300F5Vhas a planet (b)
BH CruBH59844 12h 16m 16.79s−56° 17 09.67.968200SC4.5-7/8eMira variable, Vmax = +6.6m, Vmin = +9.8m, P = 530 d
X CruX110945 12h 46m 22.27s−59° 07 29.18.10G1IbCepheid variable, Vmax = +8.1m, Vmin = +8.7m, P = 6.21997 d
W CruW10599859483 12h 11m 59.16s−58° 47 00.78.44G2Iabβ Lyr variable
AB CruAB10687159935 12h 17m 37.12s−58° 09 52.48.483900B2IVeAlgol variable
AI CruAI59026 12h 06m 07.69s−61° 15 24.89.682300F7Ib-IIAlgol variable
GX 301-2BP 12h 26m 37.56s−62° 46 13.210.66B1.2IaHigh-mass X-ray binary, Vmax = +10.4m, Vmin = +10.92m, P = 41.487 d
WR 46DI10499458954 12h 05m 18.72s−62° 03 10.110.8−2.2513000WN3pWolf–Rayet star, Vmax = +10.49m, Vmin = +11.00m
HDE 311884CD311884 12h 43m 51.00s−63° 45 14.810.81911WN6o + O5VWolf–Rayet star, ΔV = 0.11m, P = 6.24 d
NGC 4349-127 12h 24m 35.47s−61° 49 11.710.826500KIIIhas a planet
BI CruBI 12h 23m 25.99s−62° 38 16.111.00B+....Symbiotic star, Vmax = +11.0m, Vmin = +14.0m
Table legend:

See also

Notes

  1. Preibisch, T., Mamajek, E. (2008). "The Nearest OB Association: Scorpius-Centaurus (Sco OB2)". Handbook of Star-Forming Regions. 2: 0. arXiv:0809.0407. Bibcode:2008hsf2.book..235P.CS1 maint: multiple names: authors list (link)
  2. "IAU Catalog of Star Names". International Astronomical Union. Retrieved 2018-09-17.
  3. de Zeeuw, P.T.; Hoogerwerf, R.; de Bruijne, J.H.J.; Brown, A.G.A.; Blaauw, A. (1999). "A Hipparcos Census of Nearby OB Associations". Astronomical Journal. 117 (1): 354–99. arXiv:astro-ph/9809227. Bibcode:1999AJ....117..354D. doi:10.1086/300682.

References

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