# Llista d'estrelles dels Llebrers

La llista d'estrelles dels Llebrers pretén recollir de forma sintètica i mostrant algunes poques de les seves principals característiques de les estrelles notables de la Constel·lació dels Llebrers, ordenades, a priori, per ordre decreixent de brillantor.
| Nom | B | F | Var | HD | HIP | RA | Dec | mag. ap. | mag. abs. | Dist. (al) | Tipus sp. | Notes |
| Cor Caroli | α² | 12 | | 112413 | 63125 | 12$^h$ 56$^m$ 01.84$^s$ | +38° 19′ 05.7″ | 2.89 | 0.25 | 114 | A0spe... | prototipus de variable α² CVn, V$_{max}$ = 2.86$^m$, V$_{min}$ = 2.93$^m$, P = 5.46939 d; estrella binària amb α¹ CVn |
| β CVn | β | 8 | | 109358 | 61317 | 12$^h$ 33$^m$ 45.09$^s$ | +41° 21′ 24.4″ | 4.24 | 4.63 | 27 | G0V | Chara, Asterion; anàleg solar; es sospita que és una estrella variable, V$_{max}$ = 4.24$^m$, V$_{min}$ = 4.29$^m$ |
| 24 CVn | | 24 | | 118232 | 66234 | 13$^h$ 34$^m$ 27.37$^s$ | +49° 00′ 57.3″ | 4.68 | 0.85 | 190 | A5V | es sospita que és una estrella variable, V$_{max}$ = 4.60$^m$, V$_{min}$ = 4.70$^m$ |
| 20 CVn | | 20 | AO | 115604 | 64844 | 13$^h$ 17$^m$ 32.64$^s$ | +40° 34′ 21.2″ | 4.72 | 0.00 | 286 | F3III | variable δ Sct, V$_{max}$ = 4.7$^m$, V$_{min}$ = 4.75$^m$, P = 0.12168 d |
| AW CVn | | | AW | 120933 | 67665 | 13$^h$ 51$^m$ 47.49$^s$ | +34° 26′ 39.5″ | 4.76 | −1.58 | 604 | K5III | variable semiregular, V$_{max}$ = 4.72$^m$, V$_{min}$ = 4.81$^m$ |
| 5 CVn | | 5 | | 107950 | 60485 | 12$^h$ 24$^m$ 01.48$^s$ | +51° 33′ 44.0″ | 4.77 | −0.64 | 393 | G7III | es sospita que és binària eclipsant, ΔV = 0.07$^m$ |
| 25 CVn | | 25 | | 118623 | 66458 | 13$^h$ 37$^m$ 27.70$^s$ | +36° 17′ 41.4″ | 4.82 | 0.97 | 192 | A7III | estrella binària |
| HR 5110 | | | BH | 118216 | 66257 | 13$^h$ 34$^m$ 47.75$^s$ | +37° 10′ 56.8″ | 4.91 | 1.67 | 145 | F2IV SB | variable RS CVn, ΔV = 0.07$^m$, P = 2.61317 d |
| HD 115004 | | | | 115004 | 64540 | 13$^h$ 13$^m$ 42.98$^s$ | +40° 09′ 10.3″ | 4.94 | −1.08 | 522 | K0III | |
| 6 CVn | | 6 | | 108225 | 60646 | 12$^h$ 25$^m$ 51.00$^s$ | +39° 01′ 07.3″ | 5.01 | 0.79 | 227 | G8III-IV | estrella variable, ΔV = 0.006$^m$, P = 157.23270 d |
| 21 CVn | | 21 | BK | 115735 | 64906 | 13$^h$ 18$^m$ 14.54$^s$ | +49° 40′ 55.3″ | 5.13 | 0.51 | 275 | A0V | variable α² CVn, ΔV = 0.04$^m$ |
| 14 CVn | | 14 | | 113797 | 63901 | 13$^h$ 05$^m$ 44.46$^s$ | +35° 47′ 55.9″ | 5.20 | 0.51 | 282 | B9V | es sospita que és una estrella variable, V$_{max}$ = 5.10$^m$, V$_{min}$ = 5.29$^m$ |
| 3 CVn | | 3 | | 107274 | 60122 | 12$^h$ 19$^m$ 48.72$^s$ | +48° 59′ 02.9″ | 5.28 | −0.72 | 517 | M0III | es sospita que és una estrella variable |
| HD 109317 | | | | 109317 | 61309 | 12$^h$ 33$^m$ 38.90$^s$ | +33° 14′ 51.6″ | 5.42 | 0.86 | 266 | K0IIICN... | |
| La Superba | | | Y | 110914 | 62223 | 12$^h$ 45$^m$ 07.83$^s$ | +45° 26′ 24.8″ | 5.42 | −1.27 | 710 | C7Iab | variable semiregular, V$_{max}$ = 4.86$^m$, V$_{min}$ = 5.88$^m$, P = 267.8 d |
| HD 120164 | | | | 120164 | 67250 | 13$^h$ 46$^m$ 59.87$^s$ | +38° 32′ 33.9″ | 5.51 | 0.67 | 304 | K0III+... | |
| 23 CVn | | 23 | | 116010 | 65072 | 13$^h$ 20$^m$ 19.00$^s$ | +40° 09′ 02.0″ | 5.60 | −0.91 | 655 | K1III | |
| α¹ CVn | α¹ | 12 | | 112412 | 63121 | 12$^h$ 56$^m$ 00.60$^s$ | +38° 18′ 52.9″ | 5.61 | | 120.2 | F0V | forma part del sistema Cor Caroli |
| HD 120420 | | | | 120420 | 67384 | 13$^h$ 48$^m$ 38.74$^s$ | +31° 11′ 24.4″ | 5.61 | 0.71 | 311 | K0III | |
| HD 113847 | | | | 113847 | 63916 | 13$^h$ 05$^m$ 52.28$^s$ | +45° 16′ 06.6″ | 5.64 | −0.21 | 483 | K1III | es sospita que és una estrella variable, V$_{max}$ = 5.64$^m$, V$_{min}$ = 5.84$^m$ |
| 2 CVn | | 2 | | 106690 | 59831 | 12$^h$ 16$^m$ 07.54$^s$ | +40° 39′ 36.9″ | 5.69 | −1.35 | 834 | M1III | |
| TU CVn | | | TU | 112264 | 63024 | 12$^h$ 54$^m$ 56.54$^s$ | +47° 11′ 48.3″ | 5.75 | −0.92 | 704 | M5III | variable semiregular, V$_{max}$ = 5.50$^m$, V$_{min}$ = 6.2$^m$, P = 44.2 d |
| 19 CVn | | 19 | | 115271 | 64692 | 13$^h$ 15$^m$ 32.05$^s$ | +40° 51′ 18.6″ | 5.77 | 1.39 | 245 | A7V | |
| HD 115723 | | | | 115723 | 64927 | 13$^h$ 18$^m$ 27.71$^s$ | +34° 05′ 53.9″ | 5.81 | −0.14 | 504 | K4.5III | |
| HD 111604 | | | DT | 111604 | 62641 | 12$^h$ 50$^m$ 10.81$^s$ | +37° 31′ 00.8″ | 5.87 | 0.50 | 387 | A3V | variable δ Sct |
| HD 116957 | | | | 116957 | 65550 | 13$^h$ 26$^m$ 16.58$^s$ | +46° 01′ 41.2″ | 5.88 | 0.68 | 357 | K0III: | |
| HD 120047 | | | | 120047 | 67194 | 13$^h$ 46$^m$ 13.63$^s$ | +41° 05′ 19.9″ | 5.88 | 2.33 | 167 | A5V | |
| HD 120819 | | | | 120819 | 67605 | 13$^h$ 51$^m$ 09.21$^s$ | +34° 39′ 52.3″ | 5.89 | −0.69 | 676 | M2III | estrella variable, ΔV = 0.010$^m$, P = 7.94786 d |
| 17 CVn | | 17 | | 114447 | 64246 | 13$^h$ 10$^m$ 03.27$^s$ | +38° 29′ 55.9″ | 5.91 | 1.95 | 202 | A9III-IV | variable γ Dor, ΔV = 0.008$^m$, P = 0.69004 d |
| HD 121164 | | | | 121164 | 67782 | 13$^h$ 53$^m$ 10.36$^s$ | +28° 38′ 53.0″ | 5.91 | 1.86 | 211 | A7V | |
| HD 120048 | | | | 120048 | 67210 | 13$^h$ 46$^m$ 19.10$^s$ | +38° 30′ 13.2″ | 5.92 | 0.46 | 403 | G9III | |
| 10 CVn | | 10 | | 110897 | 62207 | 12$^h$ 44$^m$ 59.68$^s$ | +39° 16′ 42.9″ | 5.95 | 4.75 | 57 | G0V | |
| HD 119458 | | | | 119458 | 66907 | 13$^h$ 42$^m$ 43.42$^s$ | +34° 59′ 20.4″ | 5.98 | 0.11 | 486 | G5III | |
| HD 114357 | | | | 114357 | 64212 | 13$^h$ 09$^m$ 38.72$^s$ | +37° 25′ 23.3″ | 6.01 | 1.20 | 299 | K3III | |
| HD 115810 | | | | 115810 | 64979 | 13$^h$ 19$^m$ 04.27$^s$ | +35° 07′ 40.6″ | 6.01 | 1.94 | 213 | F0IV | |
| 4 CVn | | 4 | AI | 107904 | 60467 | 12$^h$ 23$^m$ 47.08$^s$ | +42° 32′ 33.8″ | 6.03 | 0.98 | 334 | F3IV | variable δ Sct, V$_{max}$ = 5.89$^m$, V$_{min}$ = 6.15$^m$, P = 0.2085 d |
| HD 117710 | | | | 117710 | 65951 | 13$^h$ 31$^m$ 15.84$^s$ | +42° 06′ 21.9″ | 6.07 | 1.53 | 263 | K2III | |
| CL CVn | | | CL | 116581 | 65376 | 13$^h$ 23$^m$ 53.92$^s$ | +37° 02′ 02.2″ | 6.10 | −1.74 | 1207 | M3III | variable irregular lenta, ΔV = ~0.10$^m$ |
| HD 112570 | | | | 112570 | 63211 | 12$^h$ 57$^m$ 07.80$^s$ | +46° 10′ 36.9″ | 6.12 | 0.99 | 344 | K0III-IV | es sospita que és una estrella variable, V$_{max}$ = 6.12$^m$, V$_{min}$ = 6.5$^m$ |
| 7 CVn | | 7 | | 108845 | 60988 | 12$^h$ 30$^m$ 03.10$^s$ | +51° 32′ 08.1″ | 6.21 | 2.94 | 147 | F7V | |
| HD 119035 | | | | 119035 | 66690 | 13$^h$ 40$^m$ 15.63$^s$ | +31° 00′ 42.5″ | 6.21 | 0.12 | 540 | G5II: | |
| HD 119081 | | | | 119081 | 66725 | 13$^h$ 40$^m$ 39.12$^s$ | +28° 03′ 54.5″ | 6.22 | 0.88 | 382 | K3III | |
| HD 109345 | | | | 109345 | 61320 | 12$^h$ 33$^m$ 47.41$^s$ | +33° 23′ 04.9″ | 6.24 | 0.94 | 374 | K0III | |
| 11 CVn | | 11 | | 111421 | 62516 | 12$^h$ 48$^m$ 41.86$^s$ | +48° 28′ 00.5″ | 6.25 | 0.49 | 463 | A6m | |
| HD 112171 | | | | 112171 | 62972 | 12$^h$ 54$^m$ 13.15$^s$ | +33° 32′ 03.9″ | 6.25 | 1.89 | 243 | A7IV | |
| 15 CVn | | 15 | | 114376 | 64217 | 13$^h$ 09$^m$ 42.04$^s$ | +38° 32′ 01.9″ | 6.25 | −1.48 | 1144 | B7III | |
| HD 122675 | | | | 122675 | 68567 | 14$^h$ 02$^m$ 12.17$^s$ | +45° 45′ 13.1″ | 6.28 | 0.17 | 544 | K2III | |
| HD 119445 | | | | 119445 | 66892 | 13$^h$ 42$^m$ 28.87$^s$ | +41° 40′ 27.3″ | 6.30 | −1.00 | 942 | G6III | |
| HD 121682 | | | | 121682 | 68065 | 13$^h$ 56$^m$ 10.54$^s$ | +32° 01′ 56.9″ | 6.31 | 2.01 | 236 | F4IV-V | |
| HD 107610 | | | | 107610 | 60305 | 12$^h$ 21$^m$ 56.30$^s$ | +47° 10′ 56.1″ | 6.33 | 1.46 | 307 | K2III | |
| HD 110834 | | | | 110834 | 62172 | 12$^h$ 44$^m$ 27.12$^s$ | +44° 06′ 10.8″ | 6.34 | 1.54 | 298 | F6IV | |
| HD 116303 | | | | 116303 | 65230 | 13$^h$ 22$^m$ 03.97$^s$ | +43° 54′ 12.0″ | 6.34 | 0.60 | 458 | A7m | es sospita que és una estrella variable, V$_{max}$ = 6.34$^m$, V$_{min}$ = 6.37$^m$ |
| 9 CVn | | 9 | | 109980 | 61692 | 12$^h$ 38$^m$ 46.30$^s$ | +40° 52′ 28.9″ | 6.35 | 2.27 | 213 | A7Vn | es sospita que és una estrella variable |
| HD 118156 | | | | 118156 | 66223 | 13$^h$ 34$^m$ 21.85$^s$ | +38° 47′ 21.2″ | 6.37 | 2.20 | 223 | F0IV | |
| HD 110066 | | | AX | 110066 | 61748 | 12$^h$ 39$^m$ 16.85$^s$ | +35° 57′ 07.1″ | 6.39 | 0.44 | 505 | A0p SrCrEu | variable α² CVn, V$_{max}$ = 6.32$^m$, V$_{min}$ = 6.55$^m$, P = 4900 d |
| HD 117361 | | | | 117361 | 65754 | 13$^h$ 28$^m$ 45.80$^s$ | +50° 43′ 07.5″ | 6.42 | 1.97 | 253 | F0IV | |
| HD 120600 | | | | 120600 | 67483 | 13$^h$ 49$^m$ 44.98$^s$ | +36° 37′ 58.0″ | 6.43 | 2.37 | 212 | A7IV-V | |
| HD 121197 | | | | 121197 | 67778 | 13$^h$ 53$^m$ 08.44$^s$ | +40° 20′ 16.8″ | 6.48 | −1.64 | 1370 | K5 | |
| HD 117261 | | | | 117261 | 65723 | 13$^h$ 28$^m$ 26.23$^s$ | +40° 43′ 47.2″ | 6.49 | 0.88 | 432 | G8III | |
| HD 111572 | | | | 111572 | 62600 | 12$^h$ 49$^m$ 38.05$^s$ | +48° 44′ 24.2″ | 6.50 | 0.58 | 497 | K1III | es sospita que és una estrella variable, V$_{max}$ = 6.47$^m$, V$_{min}$ = 6.53$^m$ |
| HD 114975 | | | | 114975 | 64530 | 13$^h$ 13$^m$ 35.94$^s$ | +36° 53′ 15.3″ | 6.50 | −1.58 | 1347 | M0 | |
| V CVn | | | V | 115898 | 65006 | 13$^h$ 19$^m$ 27.77$^s$ | +45° 31′ 37.7″ | 6.74 | | 2260 | M6IIIa | variable semiregular, V$_{max}$ = 6.52$^m$, V$_{min}$ = 8.56$^m$, P = 191.89 d |
| HD 108100 | | | DD | 108100 | 60571 | 12$^h$ 24$^m$ 13.93$^s$ | +42° 51′ 17.0″ | 7.15 | | 267.4 | F2V | variable γ Dor, ΔV = 0.04$^m$, P = 0.754307 d |
| BM CVn | | | BM | 116204 | 65187 | 13$^h$ 21$^m$ 32.26$^s$ | +38° 52′ 49.5″ | 7.21 | | 368 | K2III | variable RS CVn, ΔV = 0.06$^m$, P = 21.7 d |
| R CVn | | | R | 120499 | 67410 | 13$^h$ 48$^m$ 57.20$^s$ | +39° 32′ 34.0″ | 7.40 | | 3130 | M6IIIe | variable Mira, V$_{max}$ = 6.5$^m$, V$_{min}$ = 12.9$^m$, P = 328.53 d |
| HD 109995 | | | | 109995 | 61696 | 12$^h$ 38$^m$ 47.60$^s$ | +39° 18′ 31.6″ | 7.64 | | 891 | A0p | estrella de la branca horitzontal |
| HD 115781 | | | BL | 115781 | 64956 | 13$^h$ 18$^m$ 51.94$^s$ | +33° 26′ 19.3″ | 8.13 | | 691 | K1III | variable elipsoidal rotant, ΔV = 0.24$^m$, P = 18.692 d |
| RS CVn | | | RS | 114519 | 64293 | 13$^h$ 10$^m$ 36.91$^s$ | +35° 56′ 05.6″ | 8.23 | | 352 | F4V+... | prototipus de variable RS CVn, V$_{max}$ = 7.93$^m$, V$_{min}$ = 9.14$^m$, P = 4.797887 d |
| TT CVn | | | TT | 112869 | 63389 | 12$^h$ 59$^m$ 22.64$^s$ | +37° 49′ 03.7″ | 8.91 | | | Rp... | variable semiregular |
| HD 115444 | | | | 115444 | 64786 | 13$^h$ 16$^m$ 42.46$^s$ | +36° 22′ 52.7″ | 8.97 | | 918 | G9V | estel de bari |
| TX CVn | | | TX | | | 12$^h$ 44$^m$ 22.07$^s$ | +36° 45′ 50.7″ | 9.34 | | | B1-B9Veq + K0III-M4 | Z And i variable elipsoidal rotant, V$_{max}$ = 9.34$^m$, V$_{min}$ = 10.28$^m$, P = 199.75 d |
| VZ CVn | | | VZ | 117777 | 66017 | 13$^h$ 32$^m$ 03.39$^s$ | +28° 35′ 04.9″ | 9.35 | | 1460 | F3V + F6V | variable Algol i varialbe γ Dor, V$_{max}$ = 9.17$^m$, V$_{min}$ = 9.72$^m$, P = 0.84246163 d |
| Gliese 521 | | | | | 66625 | 13$^h$ 39$^m$ 24.10$^s$ | +46° 11′ 11.4″ | 10.26 | | 42.41 | M2.0V | possiblement té un planeta (b) |
| BI CVn | | | BI | | 63701 | 13$^h$ 03$^m$ 16.41$^s$ | +36° 37′ 00.6″ | 10.31 | | 782 | F9V | variable W UMa, V$_{max}$ = 10.26$^m$, V$_{min}$ = 10.71$^m$, P = 0.38416 d |
| W CVn | | | W | | 68908 | 14$^h$ 06$^m$ 27.98$^s$ | +37° 49′ 41.5″ | 10.49 | | 4900 | F2III | variable RR Lyr, V$_{max}$ = 10.03$^m$, V$_{min}$ = 10.96$^m$, P = 0.5517588 d |
| Gliese 490 | | | BF | | 63253 | 12$^h$ 57$^m$ 40.26$^s$ | +35° 13′ 30.0″ | 10.52 | | 62.78 | M0.0V | estrella binària; variable BY Dra i estrella fulgurant, V$_{max}$ = 10.5$^m$, V$_{min}$ = 10.6$^m$, P = 3.17 d |
| ST CVn | | | ST | | 68188 | 13$^h$ 57$^m$ 34.06$^s$ | +29° 51′ 28.7″ | 11.21 | | | A1 | variable RR Lyr, V$_{max}$ = 11.04$^m$, V$_{min}$ = 11.6$^m$, P = 0.329045 d |
| UZ CVn | | | UZ | | 61029 | 12$^h$ 30$^m$ 27.70$^s$ | +40° 30′ 32.0″ | 12.11 | | 964 | A8 | variable RR Lyr |
| Z CVn | | | Z | | | 12$^h$ 49$^m$ 45.37$^s$ | +43° 46′ 25.1″ | 12.12 | | | A5 | variable RR Lyr, V$_{max}$ = 11.46$^m$, V$_{min}$ = 12.36$^m$, P = 0.653819 d |
| DG CVn | | | DG | | | 13$^h$ 31$^m$ 46.62$^s$ | +29° 16′ 36.7″ | 12.19 | | 25.9 | M4.0V | estrella fulgurant i variable BY Dra |
| HAT-P-36 | | | | | | 12$^h$ 33$^m$ 03$^s$ | +44° 54′ 55″ | 12.26 | | 1034 | | té un planeta en trànsit (b) |
| UX CVn | | | UX | | | 12$^h$ 14$^m$ 48.54$^s$ | +36° 38′ 49.3″ | | | | B2 | variable elipsoidal rotant i binària eclipsant |
| HAT-P-12 | | | | | | 13$^h$ 57$^m$ 33.48$^s$ | +43° 29′ 36.7″ | 12.84 | | | K5 | té un planeta en trànsit |
| AM CVn | | | AM | | | 12$^h$ 34$^m$ 54.60$^s$ | +37° 37′ 44.1″ | 14.18 | | 330 | DBp | prototipus d'estrella AM CVn |
| GD 154 | | | BG | | | 13$^h$ 09$^m$ 57.69$^s$ | +35° 09′ 47.1″ | 15.33 | | | DA4.4 | variable ZZ Cet, ΔV = 0.09$^m$, P = 0.013727 d |

## Vegeu també

* Llista d'estrelles per constel·lació

## Referències

* ESA. «The Hipparcos and Tycho Catalogues», 1997. [Consulta: 5 gener 2015].
* Gould, B. A. «Uranometria Argentina». Reprinted and updated by Pilcher, F. Arxivat de l'original el 2012-02-27. [Consulta: 5 gener 2015].
* Kostjuk, N. D. «HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index», 2002. [Consulta: 5 gener 2015].
* Roman, N. G. «Identification of a Constellation from a Position», 1987. [Consulta: 5 gener 2015].