# List of stars in Monoceros

This is the list of notable stars in the constellation Monoceros, sorted by decreasing brightness.
| Name | B | F | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| α Mon | α | 26 | | 61935 | 37447 | 07$^h$ 41$^m$ 14.88$^s$ | −09° 33′ 03.9″ | 3.94 | 0.71 | 144 | K0III | |
| γ Mon | γ | 5 | | 43232 | 29651 | 06$^h$ 14$^m$ 51.34$^s$ | −06° 16′ 29.0″ | 3.99 | −2.49 | 644 | K3III | |
| δ Mon | δ | 22 | | 55185 | 34769 | 07$^h$ 11$^m$ 51.86$^s$ | −00° 29′ 34.0″ | 4.15 | −1.15 | 375 | A2V | |
| ζ Mon | ζ | 29 | | 67594 | 39863 | 08$^h$ 08$^m$ 35.66$^s$ | −02° 59′ 01.6″ | 4.36 | −4.41 | 1852 | G2Ib | |
| ε Mon A | ε | 8 | | 44769 | 30419 | 06$^h$ 23$^m$ 46.10$^s$ | +04° 35′ 34.2″ | 4.39 | 1.41 | 128 | A5IV | component of the ε Mon system |
| 13 Mon | | 13 | | 46300 | 31216 | 06$^h$ 32$^m$ 54.23$^s$ | +07° 19′ 58.7″ | 4.47 | −3.86 | 1509 | A0Ib | suspected variable |
| 18 Mon | | 18 | | 49293 | 32578 | 06$^h$ 47$^m$ 51.66$^s$ | +02° 24′ 43.9″ | 4.48 | −0.81 | 373 | K0III | |
| β Mon A | β | 11 | | 45725 | 30867 | 06$^h$ 28$^m$ 49.07$^s$ | −07° 01′ 59.0″ | 4.60 | −2.03 | 691 | B3Ve | Herschel's Wonder Star; component of the β Mon system; Be star |
| S Mon | | 15 | S | 47839 | 31978 | 06$^h$ 40$^m$ 58.66$^s$ | +09° 53′ 44.7″ | 4.66 | −2.82 | 1022 | O7V + O9.5V | in NGC 2264; irregular variable, V$_{max}$ = 4.62$^m$, V$_{min}$ = 4.68$^m$ |
| 28 Mon | | 28 | V645 | 65953 | 39211 | 08$^h$ 01$^m$ 13.30$^s$ | −01° 23′ 32.7″ | 4.68 | −1.12 | 472 | K4III | FK Com variable, ΔV = 0.02$^m$, P = 0.21 d |
| 17 Mon | | 17 | | 49161 | 32533 | 06$^h$ 47$^m$ 19.84$^s$ | +08° 02′ 14.2″ | 4.77 | −1.09 | 484 | K4III | |
| 20 Mon | | 20 | | 54810 | 34622 | 07$^h$ 10$^m$ 13.68$^s$ | −04° 14′ 15.5″ | 4.91 | 0.85 | 211 | K0III | |
| 3 Mon | | 3 | | 40967 | 28574 | 06$^h$ 01$^m$ 50.43$^s$ | −10° 35′ 52.6″ | 4.92 | −2.47 | 979 | B5III | suspected variable |
| 27 Mon | | 27 | | 65695 | 39079 | 07$^h$ 59$^m$ 44.18$^s$ | −03° 40′ 46.5″ | 4.93 | 0.51 | 250 | K2III | |
| 19 Mon | | 19 | V637 | 52918 | 33971 | 07$^h$ 02$^m$ 54.78$^s$ | −04° 14′ 21.3″ | 4.99 | −2.68 | 1116 | B1V | β Cep variable, V$_{max}$ = 4.96$^m$, V$_{min}$ = 5.01$^m$, P = 0.19 d |
| 2 Mon | | 2 | | 40536 | 28325 | 05$^h$ 59$^m$ 04.31$^s$ | −09° 33′ 29.3″ | 5.04 | 0.02 | 328 | A6m | |
| HD 42690 | | | | 42690 | 29417 | 06$^h$ 11$^m$ 51.82$^s$ | −06° 33′ 01.0″ | 5.06 | −2.78 | 1203 | B2V | |
| 10 Mon | | 10 | | 45546 | 30772 | 06$^h$ 27$^m$ 57.57$^s$ | −04° 45′ 43.7″ | 5.06 | −3.03 | 1353 | B2V | |
| HD 49331 | | | | 49331 | 32558 | 06$^h$ 47$^m$ 37.22$^s$ | −08° 59′ 54.6″ | 5.08 | −2.94 | 1309 | M1II | suspected variable, V$_{max}$ = 5.00$^m$, V$_{min}$ = 5.11$^m$ |
| HD 46487 | | | | 46487 | 31278 | 06$^h$ 33$^m$ 37.92$^s$ | −01° 13′ 12.4″ | 5.09 | −0.99 | 536 | B5Vn | |
| 25 Mon | | 25 | | 61064 | 37088 | 07$^h$ 37$^m$ 16.73$^s$ | −04° 06′ 39.7″ | 5.13 | 1.18 | 202 | F6III | suspected δ Sct variable, ΔV = 0.01$^m$ |
| HR 2142 | | | V696 | 41335 | 28744 | 06$^h$ 04$^m$ 13.50$^s$ | −06° 42′ 32.2″ | 5.19 | −2.06 | 918 | B2Vne+ | unique variable |
| 77 Ori | | (77) | | 45416 | 30717 | 06$^h$ 27$^m$ 13.76$^s$ | +00° 17′ 57.4″ | 5.19 | −2.13 | 950 | K1II | |
| HD 48217 | | | | 48217 | 32064 | 06$^h$ 41$^m$ 56.37$^s$ | −09° 10′ 02.7″ | 5.21 | −0.11 | 378 | M0III | |
| HD 52666 | | | | 52666 | 33878 | 07$^h$ 01$^m$ 56.39$^s$ | −05° 43′ 19.5″ | 5.21 | −1.38 | 682 | M2III | suspected variable, V$_{max}$ = 5.15$^m$, V$_{min}$ = 5.21$^m$ |
| HD 46089 | | | | 46089 | 31119 | 06$^h$ 31$^m$ 48.29$^s$ | +11° 32′ 39.6″ | 5.22 | 1.16 | 211 | A3V | |
| 7 Mon | | 7 | | 44112 | 30073 | 06$^h$ 19$^m$ 42.80$^s$ | −07° 49′ 22.5″ | 5.27 | −1.74 | 823 | B2.5V | |
| HD 43993 | | | | 43993 | 29996 | 06$^h$ 18$^m$ 50.58$^s$ | −09° 23′ 23.9″ | 5.36 | −0.62 | 511 | K1III | |
| HD 41692 | | | | 41692 | 28949 | 06$^h$ 06$^m$ 38.74$^s$ | −04° 11′ 37.8″ | 5.37 | −3.71 | 2131 | B5IV | |
| β Mon B | β | 11 | | 45726 | | 06$^h$ 28$^m$ 49.50$^s$ | −07° 02′ 04.0″ | 5.40 | | | | Herschel's Wonder Star; component of the β Mon system |
| HD 46229 | | | | 46229 | 31121 | 06$^h$ 31$^m$ 50.07$^s$ | −08° 09′ 29.5″ | 5.43 | −1.70 | 869 | K2III | |
| 21 Mon | | 21 | V571 | 55057 | 34724 | 07$^h$ 11$^m$ 23.63$^s$ | −00° 18′ 06.9″ | 5.44 | 0.92 | 261 | F2V | δ Sct variable, V$_{max}$ = 5.43$^m$, V$_{min}$ = 5.5$^m$, P = 0.089 d |
| HD 50747 | | | | 50747 | 33184 | 06$^h$ 54$^m$ 24.66$^s$ | −01° 07′ 37.1″ | 5.45 | −0.42 | 484 | A4IV | γ Dor variable, ΔV = 0.001$^m$, P = 0.21 d |
| HD 62902 | | | | 62902 | 37901 | 07$^h$ 46$^m$ 02.16$^s$ | −06° 46′ 20.2″ | 5.49 | 1.17 | 238 | K5III | |
| HD 47054 | | | | 47054 | 31583 | 06$^h$ 36$^m$ 35.33$^s$ | −05° 12′ 40.0″ | 5.52 | −1.52 | 834 | B8V | |
| 78 Ori | | (78) | | 45433 | 30720 | 06$^h$ 27$^m$ 15.59$^s$ | −00° 16′ 33.6″ | 5.55 | −1.26 | 749 | K5III | |
| HD 45415 | | | | 45415 | 30728 | 06$^h$ 27$^m$ 20.48$^s$ | +02° 54′ 29.7″ | 5.55 | 0.79 | 292 | G9III | |
| β Mon C | β | | | 45727 | | 06$^h$ 28$^m$ 49.50$^s$ | −07° 02′ 04.0″ | 5.60 | | | | Herschel's Wonder Star; component of the β Mon system |
| HD 46304 | | | | 46304 | 31167 | 06$^h$ 32$^m$ 23.13$^s$ | −05° 52′ 07.4″ | 5.60 | 2.42 | 141 | F0Vnn+... | |
| HD 59311 | | | | 59311 | 36388 | 07$^h$ 29$^m$ 18.68$^s$ | −01° 54′ 19.1″ | 5.60 | −2.89 | 1630 | K5III | |
| HD 63752 | | | | 63752 | 38253 | 07$^h$ 50$^m$ 10.58$^s$ | −09° 11′ 00.4″ | 5.60 | −2.57 | 1405 | K3III | |
| HD 53208 | | | | 53208 | 34086 | 07$^h$ 04$^m$ 05.25$^s$ | −05° 19′ 26.3″ | 5.63 | −2.38 | 1304 | K3III | suspected variable |
| HD 49147 | | | | 49147 | 32474 | 06$^h$ 46$^m$ 39.02$^s$ | −10° 06′ 26.5″ | 5.66 | −0.42 | 535 | B9.5V | |
| HD 49434 | | | | 49434 | 32617 | 06$^h$ 48$^m$ 19.09$^s$ | −01° 19′ 07.8″ | 5.75 | 2.74 | 131 | F1V | δ Sct and γ Dor variable |
| HD 49643 | | | | 49643 | 32698 | 06$^h$ 49$^m$ 16.41$^s$ | −02° 16′ 19.3″ | 5.75 | −0.42 | 558 | B8IIIn | |
| HD 50277 | | | | 50277 | 33024 | 06$^h$ 52$^m$ 49.49$^s$ | +08° 22′ 49.6″ | 5.75 | 1.77 | 204 | F0Vn | |
| HD 59381 | | | | 59381 | 36396 | 07$^h$ 29$^m$ 22.11$^s$ | −10° 19′ 36.0″ | 5.75 | −1.52 | 926 | K5III | slow irregular variable, V$_{max}$ = 5.74$^m$, V$_{min}$ = 5.76$^m$ |
| HD 64235 | | | | 64235 | 38474 | 07$^h$ 52$^m$ 47.87$^s$ | −05° 25′ 41.5″ | 5.76 | 2.70 | 133 | F5IVs | suspected variable, V$_{max}$ = 5.74$^m$, V$_{min}$ = 5.77$^m$ |
| HD 46769 | | | | 46769 | 31446 | 06$^h$ 35$^m$ 15.83$^s$ | +00° 53′ 24.8″ | 5.78 | −3.94 | 2860 | B8Ib | |
| HD 49933 | | | | 49933 | 32851 | 06$^h$ 50$^m$ 49.82$^s$ | −00° 32′ 25.5″ | 5.78 | 3.40 | 97 | F2V | |
| HD 53510 | | | | 53510 | 34215 | 07$^h$ 05$^m$ 39.00$^s$ | +09° 11′ 09.0″ | 5.78 | −0.40 | 562 | M0III | variable star, ΔV = 0.007$^m$, P = 0.088 d |
| HD 47964 | | | | 47964 | 31992 | 06$^h$ 41$^m$ 05.45$^s$ | +00° 29′ 43.2″ | 5.79 | −1.96 | 1156 | B8III | |
| HD 55775 | | | | 55775 | 34975 | 07$^h$ 14$^m$ 10.87$^s$ | −03° 54′ 06.3″ | 5.80 | −0.57 | 613 | K5III | |
| U Mon | | | U | 59693 | 36521 | 07$^h$ 30$^m$ 47.47$^s$ | −09° 46′ 36.8″ | 5.82 | | 2248 | K0Ibpvar | RV Tau variable, V$_{max}$ = 5.45$^m$, V$_{min}$ = 7.67$^m$, P = 91.32 d |
| HD 43157 | | | | 43157 | 29629 | 06$^h$ 14$^m$ 36.71$^s$ | −04° 34′ 06.5″ | 5.83 | −0.56 | 617 | B5V | |
| HD 57749 | | | | 57749 | 35749 | 07$^h$ 22$^m$ 25.40$^s$ | −05° 58′ 58.1″ | 5.83 | −1.39 | 908 | F3IV | suspected δ Sct variable, V$_{max}$ = 5.80$^m$, V$_{min}$ = 5.84$^m$ |
| HD 59380 | | | | 59380 | 36399 | 07$^h$ 29$^m$ 25.61$^s$ | −07° 33′ 05.3″ | 5.86 | 3.64 | 91 | F8V | |
| HD 45320 | | | | 45320 | 30666 | 06$^h$ 26$^m$ 39.59$^s$ | −01° 30′ 26.2″ | 5.87 | 1.64 | 229 | A3Vn | |
| 12 Mon | | 12 | | 46241 | 31159 | 06$^h$ 32$^m$ 19.23$^s$ | +04° 51′ 21.6″ | 5.87 | −0.12 | 517 | K0V | suspected variable, V$_{max}$ = 5.83$^m$, V$_{min}$ = 5.87$^m$ |
| HD 41547 | | | | 41547 | 28854 | 06$^h$ 05$^m$ 27.02$^s$ | −10° 14′ 33.6″ | 5.88 | 2.03 | 192 | F4V: | γ Dor variable |
| HD 45067 | | | | 45067 | 30545 | 06$^h$ 25$^m$ 16.41$^s$ | −00° 56′ 43.3″ | 5.88 | 3.28 | 108 | F8V | |
| HD 48434 | | | | 48434 | 32226 | 06$^h$ 43$^m$ 38.65$^s$ | +03° 55′ 57.1″ | 5.88 | | 2850 | B0III | suspected β Cep variable |
| HD 51104 | | | | 51104 | 33372 | 06$^h$ 56$^m$ 25.84$^s$ | +09° 57′ 23.8″ | 5.90 | −0.28 | 561 | B8Vn | |
| HD 55832 | | | | 55832 | 34982 | 07$^h$ 14$^m$ 15.52$^s$ | −09° 56′ 51.1″ | 5.90 | −3.38 | 2345 | K3III | |
| HD 59984 | | | | 59984 | 36640 | 07$^h$ 32$^m$ 05.82$^s$ | −08° 52′ 51.3″ | 5.90 | 3.52 | 98 | F5V | suspected variable, V$_{max}$ = 5.5$^m$, V$_{min}$ = 6.8$^m$ |
| HD 45976 | | | | 45976 | 30986 | 06$^h$ 30$^m$ 11.28$^s$ | −10° 04′ 53.4″ | 5.92 | −5.50 | 6269 | K0 | |
| 16 Mon | | 16 | | 48977 | 32463 | 06$^h$ 46$^m$ 32.42$^s$ | +08° 35′ 13.8″ | 5.92 | −1.75 | 1116 | B2.5V | 53 Per variable, ΔV = 0.01$^m$, P = 1.94 d |
| HD 46709 | | | | 46709 | 31448 | 06$^h$ 35$^m$ 17.60$^s$ | +09° 59′ 18.1″ | 5.93 | −2.50 | 1583 | K4III | |
| HD 52312 | | | | 52312 | 33729 | 07$^h$ 00$^m$ 23.76$^s$ | −08° 24′ 24.6″ | 5.95 | −1.69 | 1098 | B9III | |
| HD 56207 | | | | 56207 | 35127 | 07$^h$ 15$^m$ 43.22$^s$ | −10° 35′ 01.0″ | 5.95 | 0.50 | 401 | K0 | |
| HD 51814 | | | | 51814 | 33603 | 06$^h$ 58$^m$ 57.03$^s$ | +03° 36′ 08.5″ | 5.96 | −1.31 | 926 | G8III | |
| HD 52913 | | | | 52913 | 34002 | 07$^h$ 03$^m$ 17.93$^s$ | +09° 08′ 18.1″ | 5.96 | 1.46 | 259 | A3Vs | |
| HD 58526 | | | | 58526 | 36055 | 07$^h$ 25$^m$ 51.20$^s$ | −05° 46′ 29.8″ | 5.98 | −2.84 | 1895 | G3Ib | |
| T Mon | | | T | 44990 | 30541 | 06$^h$ 25$^m$ 13.00$^s$ | +07° 05′ 08.6″ | 5.98 | | 7762 | K1Iabv SB | classical Cepheid, V$_{max}$ = 5.58$^m$, V$_{min}$ = 6.62$^m$, P = 27.02 d |
| HD 43319 | | | | 43319 | 29711 | 06$^h$ 15$^m$ 29.66$^s$ | −04° 54′ 52.7″ | 5.99 | 1.87 | 217 | A5IVs | |
| HD 61749 | | | | 61749 | 37394 | 07$^h$ 40$^m$ 35.51$^s$ | −08° 11′ 07.3″ | 6.01 | 1.12 | 310 | A3IV | |
| HD 55879 | | | | 55879 | 34999 | 07$^h$ 14$^m$ 28.26$^s$ | −10° 18′ 58.5″ | 6.02 | −3.34 | 2433 | B0III | |
| HD 50890 | | | | 50890 | 33243 | 06$^h$ 54$^m$ 58.92$^s$ | −02° 48′ 12.9″ | 6.03 | −1.90 | 1259 | G6III: | |
| Plaskett's star | | | V640 | 47129 | 31646 | 06$^h$ 37$^m$ 24.04$^s$ | +06° 08′ 07.4″ | 6.05 | −5.49 | 6618 | O8I + O7.5III | one of the most massive spectroscopic binaries known; unique variable, V$_{max}$ = 6.04$^m$, V$_{min}$ = 6.08$^m$ |
| HD 46178 | | | | 46178 | 31168 | 06$^h$ 32$^m$ 23.27$^s$ | +11° 40′ 25.0″ | 6.08 | −0.96 | 834 | K0III | |
| HD 43362 | | | | 43362 | 29705 | 06$^h$ 15$^m$ 26.16$^s$ | −09° 02′ 08.7″ | 6.09 | −0.76 | 763 | B9III | |
| HD 53929 | | | | 53929 | 34338 | 07$^h$ 07$^m$ 06.48$^s$ | +04° 54′ 38.2″ | 6.10 | −0.59 | 709 | B9.5III | |
| V721 Mon | | | V721 | 44816 | 30407 | 06$^h$ 23$^m$ 35.92$^s$ | −09° 52′ 29.1″ | 6.11 | −2.88 | 2050 | K5 | slow irregular variable |
| HD 47420 | | | | 47420 | 31733 | 06$^h$ 38$^m$ 20.46$^s$ | −02° 32′ 38.1″ | 6.14 | −0.63 | 738 | K2 | |
| 1 Mon | | 1 | V474 | 40535 | 28321 | 05$^h$ 59$^m$ 01.07$^s$ | −09° 22′ 56.1″ | 6.15 | 1.22 | 316 | F2IV | δ Sct variable |
| HD 42536 | | | V653 | 42536 | 29323 | 06$^h$ 11$^m$ 01.22$^s$ | −06° 45′ 15.1″ | 6.15 | 0.01 | 552 | A0sp... | α$^2$ CVn variable |
| HD 42278 | | | | 42278 | 29210 | 06$^h$ 09$^m$ 36.21$^s$ | −05° 42′ 41.2″ | 6.16 | 2.23 | 199 | F3IVw | |
| HD 45321 | | | | 45321 | 30660 | 06$^h$ 26$^m$ 34.45$^s$ | −04° 35′ 50.6″ | 6.16 | −1.69 | 1212 | B2.5V | |
| HD 45512 | | | | 45512 | 30804 | 06$^h$ 28$^m$ 18.80$^s$ | +10° 18′ 14.4″ | 6.16 | 1.74 | 249 | K2III-IV | |
| HR 2517 | | | V715 | 49567 | 32682 | 06$^h$ 49$^m$ 03.66$^s$ | +01° 00′ 07.5″ | 6.16 | −2.75 | 1976 | B3II-III | 53 Per variable |
| HD 63894 | | | | 63894 | 38307 | 07$^h$ 50$^m$ 55.24$^s$ | −11° 07′ 42.7″ | 6.16 | 0.66 | 411 | K0 | |
| HD 45724 | | | | 45724 | 30906 | 06$^h$ 29$^m$ 14.81$^s$ | +02° 38′ 46.6″ | 6.17 | −0.91 | 851 | M1 | suspected variable |
| HD 45995 | | | | 45995 | 31066 | 06$^h$ 31$^m$ 09.56$^s$ | +11° 15′ 05.0″ | 6.17 | −4.98 | 5525 | B2V:nne | suspected variable |
| HD 47220 | | | | 47220 | 31672 | 06$^h$ 37$^m$ 40.35$^s$ | +02° 42′ 15.4″ | 6.17 | 0.35 | 475 | K1III | |
| V638 Mon | | | V638 | 42657 | 29401 | 06$^h$ 11$^m$ 43.72$^s$ | −04° 39′ 55.6″ | 6.18 | −0.11 | 591 | B9MNp... | α$^2$ CVn variable, V$_{max}$ = 6.16$^m$, V$_{min}$ = 6.18$^m$, P = 0.72 d |
| HD 48348 | | | | 48348 | 32177 | 06$^h$ 43$^m$ 06.61$^s$ | +03° 02′ 01.8″ | 6.18 | −0.84 | 827 | K0 | |
| HD 47886 | | | | 47886 | 32012 | 06$^h$ 41$^m$ 17.22$^s$ | +11° 00′ 11.4″ | 6.19 | −3.27 | 2547 | M1III | semiregular variable |
| HD 50820 | | | | 50820 | 33210 | 06$^h$ 54$^m$ 42.04$^s$ | −01° 45′ 23.3″ | 6.20 | −4.54 | 4592 | B3IVe+... | suspected variable, V$_{max}$ = 6.16$^m$, V$_{min}$ = 6.28$^m$ |
| HD 52611 | | | | 52611 | 33873 | 07$^h$ 01$^m$ 52.91$^s$ | −01° 20′ 44.8″ | 6.20 | 0.63 | 424 | K0 | |
| V731 Mon | | | V731 | 47240 | 31697 | 06$^h$ 37$^m$ 52.70$^s$ | +04° 57′ 24.0″ | 6.20 | | 4803 | B1Ib | α Cyg variable |
| HD 44037 | | | | 44037 | 30028 | 06$^h$ 19$^m$ 07.94$^s$ | −08° 35′ 09.7″ | 6.22 | 0.78 | 399 | B9V | |
| V689 Mon | | | V689 | 47432 | 31766 | 06$^h$ 38$^m$ 38.19$^s$ | +01° 36′ 48.7″ | 6.23 | −3.86 | 3396 | O9.5II | α Cyg variable, V$_{max}$ = 6.19$^m$, V$_{min}$ = 6.26$^m$, P = 3.55 d |
| HD 54662 | | | | 54662 | 34536 | 07$^h$ 09$^m$ 20.25$^s$ | −10° 20′ 47.7″ | 6.23 | −5.03 | 5821 | O7III | |
| HD 57708 | | | | 57708 | 35737 | 07$^h$ 22$^m$ 18.59$^s$ | −02° 58′ 45.0″ | 6.23 | −0.06 | 591 | F5 | |
| HD 44783 | | | | 44783 | 30448 | 06$^h$ 24$^m$ 02.29$^s$ | +08° 53′ 06.1″ | 6.24 | −0.82 | 842 | B8Vn | |
| HD 59669 | | | | 59669 | 36526 | 07$^h$ 30$^m$ 51.14$^s$ | −05° 13′ 35.3″ | 6.24 | −5.80 | 8359 | K0 | |
| HD 51693 | | | | 51693 | 33584 | 06$^h$ 58$^m$ 38.93$^s$ | +07° 37′ 20.5″ | 6.25 | 1.93 | 238 | A3V | |
| HD 67159 | | | | 67159 | 39675 | 08$^h$ 06$^m$ 27.42$^s$ | −09° 14′ 40.1″ | 6.25 | −0.68 | 793 | B9V | |
| HD 60853 | | | | 60853 | 37000 | 07$^h$ 36$^m$ 16.67$^s$ | −08° 18′ 40.7″ | 6.27 | −0.13 | 620 | K2 | slow irregular variable, V$_{max}$ = 6.26$^m$, V$_{min}$ = 6.29$^m$ |
| HD 50931 | | | | 50931 | 33297 | 06$^h$ 55$^m$ 34.63$^s$ | +08° 19′ 27.4″ | 6.28 | 1.22 | 335 | A0V | variable star, ΔV = 0.005$^m$, P = 0.49 d |
| HD 56614 | | | | 56614 | 35301 | 07$^h$ 17$^m$ 31.68$^s$ | −06° 40′ 48.1″ | 6.29 | −2.28 | 1689 | K2 | suspected variable |
| HD 52265 | | | | 52265 | 33719 | 07$^h$ 00$^m$ 18.10$^s$ | −05° 22′ 02.5″ | 6.3 | 4.05 | 91 | G0V | Citalá, has two planets (b and c) |
| HD 44333 | | | | 44333 | 30217 | 06$^h$ 21$^m$ 25.78$^s$ | +02° 16′ 06.9″ | 6.30 | 1.25 | 334 | A4.5V | Algol variable, V$_{max}$ = 6.25$^m$, V$_{min}$ = 6.33$^m$ |
| HD 50282 | | | | 50282 | 32990 | 06$^h$ 52$^m$ 22.87$^s$ | −05° 18′ 58.5″ | 6.30 | 0.48 | 477 | K0 | |
| HD 50371 | | | | 50371 | 33082 | 06$^h$ 53$^m$ 22.40$^s$ | +10° 59′ 49.0″ | 6.30 | 0.77 | 416 | K0III | |
| HD 49976 | | | V592 | 49976 | 32838 | 06$^h$ 50$^m$ 42.31$^s$ | −08° 02′ 27.6″ | 6.31 | 1.29 | 330 | A2p SrCrEu | α$^2$ CVn variable, V$_{max}$ = 6.16$^m$, V$_{min}$ = 6.32$^m$, P = 2.98 d |
| HD 51424 | | | | 51424 | 33420 | 06$^h$ 57$^m$ 00.10$^s$ | −08° 10′ 45.4″ | 6.31 | −0.93 | 913 | A2V+... | |
| HD 67725 | | | | 67725 | 39898 | 08$^h$ 08$^m$ 56.85$^s$ | −11° 20′ 22.7″ | 6.31 | −0.44 | 729 | A0Vn | |
| HD 45168 | | | | 45168 | 30595 | 06$^h$ 25$^m$ 47.14$^s$ | −03° 53′ 20.5″ | 6.33 | −1.18 | 1035 | G9III | |
| HD 51892 | | | | 51892 | 33644 | 06$^h$ 59$^m$ 20.18$^s$ | +07° 19′ 01.2″ | 6.34 | −1.60 | 1264 | B7III | |
| HD 66242 | | | | 66242 | 39326 | 08$^h$ 02$^m$ 25.97$^s$ | −06° 20′ 13.6″ | 6.34 | 1.15 | 355 | G0III | |
| HD 45380 | | | | 45380 | 30675 | 06$^h$ 26$^m$ 44.85$^s$ | −07° 30′ 42.9″ | 6.35 | 0.86 | 409 | A0Vn | variable star, ΔV = 0.010$^m$, P = 21.97 d |
| HD 48099 | | | | 48099 | 32067 | 06$^h$ 41$^m$ 59.23$^s$ | +06° 20′ 43.5″ | 6.36 | | 2750 | O5.5V((f)) + O9V | |
| HD 50062 | | | | 50062 | 32931 | 06$^h$ 51$^m$ 39.37$^s$ | +03° 02′ 31.4″ | 6.37 | 1.57 | 298 | A2Vs | |
| HD 45090 | | | | 45090 | 30602 | 06$^h$ 25$^m$ 52.33$^s$ | +11° 07′ 33.3″ | 6.39 | 0.67 | 454 | A0 | |
| HD 47156 | | | | 47156 | 31662 | 06$^h$ 37$^m$ 36.92$^s$ | +10° 51′ 12.1″ | 6.39 | −0.77 | 883 | K0 | |
| HD 50700 | | | | 50700 | 33154 | 06$^h$ 54$^m$ 08.60$^s$ | −05° 51′ 07.9″ | 6.39 | 0.21 | 562 | A6Vn | |
| HD 45239 | | | | 45239 | 30608 | 06$^h$ 25$^m$ 58.83$^s$ | −07° 53′ 41.9″ | 6.40 | 0.24 | 556 | A4V | |
| HD 66950 | | | | 66950 | 39625 | 08$^h$ 05$^m$ 49.64$^s$ | −00° 34′ 24.0″ | 6.40 | −0.30 | 712 | K0 | suspected variable |
| HD 44700 | | | | 44700 | 30382 | 06$^h$ 23$^m$ 18.49$^s$ | +03° 45′ 52.2″ | 6.41 | −1.23 | 1098 | B3V | variable star, ΔV = 0.010$^m$, P = 31.10 d |
| V695 Mon | | | V695 | 65875 | 39172 | 08$^h$ 00$^m$ 44.14$^s$ | −02° 52′ 54.9″ | 6.42 | −3.48 | 3105 | B2.5Ve | γ Cas variable, V$_{max}$ = 6.42$^m$, V$_{min}$ = 6.53$^m$ |
| HD 45215 | | | | 45215 | 30627 | 06$^h$ 26$^m$ 09.60$^s$ | −03° 30′ 57.1″ | 6.42 | 0.34 | 536 | G5 | |
| 24 Mon | | 24 | | 56003 | 35080 | 07$^h$ 15$^m$ 19.41$^s$ | −00° 09′ 40.7″ | 6.42 | 0.36 | 530 | G5III | |
| HD 57682 | | | | 57682 | 35707 | 07$^h$ 22$^m$ 02.05$^s$ | −08° 58′ 45.9″ | 6.42 | −4.03 | 4009 | O9V | suspected variable, V$_{max}$ = 6.34$^m$, V$_{min}$ = 6.45$^m$ |
| 14 Mon | | 14 | | 46642 | 31385 | 06$^h$ 34$^m$ 46.33$^s$ | +07° 34′ 21.0″ | 6.44 | 1.21 | 362 | A0Vs | suspected variable |
| HD 53240 | | | | 53240 | 34066 | 07$^h$ 03$^m$ 57.46$^s$ | −10° 07′ 25.6″ | 6.44 | −1.52 | 1273 | B9IIIn | |
| HD 65938 | | | | 65938 | 39198 | 08$^h$ 01$^m$ 03.45$^s$ | −06° 25′ 08.7″ | 6.45 | 2.33 | 217 | G5 | |
| HD 42132 | | | | 42132 | 29140 | 06$^h$ 08$^m$ 47.72$^s$ | −06° 49′ 17.0″ | 6.46 | 1.23 | 363 | G5 | |
| HD 45563 | | | | 45563 | 30798 | 06$^h$ 28$^m$ 16.77$^s$ | +01° 54′ 45.8″ | 6.48 | 0.60 | 489 | B9V | |
| HD 52382 | | | | 52382 | 33754 | 07$^h$ 00$^m$ 39.34$^s$ | −09° 12′ 10.7″ | 6.49 | −3.28 | 2937 | B1Ib | suspected variable, V$_{max}$ = 6.47$^m$, V$_{min}$ = 6.5$^m$ |
| 9 Mon | | 9 | | 45418 | 30700 | 06$^h$ 27$^m$ 00.88$^s$ | −04° 21′ 20.3″ | 6.50 | −1.10 | 1079 | B4V | |
| V569 Mon | | | V569 | 53755 | 34234 | 07$^h$ 05$^m$ 49.64$^s$ | −10° 39′ 36.3″ | 6.50 | −3.68 | 3543 | B0.5IVn | β Cep variable, V$_{max}$ = 6.42$^m$, V$_{min}$ = 6.53$^m$, P = 0.27 d |
| IM Mon | | | IM | 44701 | 30351 | 06$^h$ 23$^m$ 01.47$^s$ | −03° 16′ 37.1″ | 6.54 | | 991 | B5V | β Lyr variable |
| HD 50281A | | | | 50281 | 32984 | 06$^h$ 52$^m$ 18.05$^s$ | −05° 10′ 25.4″ | 6.57 | | 28.395 | K3.5V | component of the HD 50281 system |
| V926 Mon | | | V926 | 52690 | 33891 | 07$^h$ 02$^m$ 06.73$^s$ | −03° 45′ 17.4″ | 6.62 | | 1920 | M1Ib | semiregular variable, V$_{max}$ = 6.50$^m$, V$_{min}$ = 6.70$^m$, P = 39 d |
| HD 50138 | | | V743 | 50138 | 32923 | 06$^h$ 51$^m$ 33.40$^s$ | −06° 57′ 59.5″ | 6.67 | | 1280 | B9e | FS CMa variable, V$_{max}$ = 6.53$^m$, V$_{min}$ = 6.87$^m$ |
| ε Mon B | ε | | | 44770 | 30422 | 06$^h$ 23$^m$ 46.50$^s$ | +04° 35′ 45.1″ | 6.72 | 4.79 | 79 | F5V | component of the ε Mon system |
| HD 46150 | | | | 46150 | 31130 | 06$^h$ 31$^m$ 55.52$^s$ | +04° 56′ 34.3″ | 6.75 | | 5200 | O5V((f)) | in NGC 2244; variable star, ΔV = 0.008$^m$ |
| 6 Mon | | 6 | | 43760 | 29885 | 06$^h$ 17$^m$ 35.13$^s$ | −10° 43′ 30.0″ | 6.76 | −0.87 | 1094 | F0e... | |
| AX Mon | | | AX | 45910 | 31019 | 06$^h$ 30$^m$ 32.94$^s$ | +05° 52′ 01.2″ | 6.85 | | 12000 | B2IIIe | unique variable, V$_{max}$ = 6.59$^m$, V$_{min}$ = 6.94$^m$, P = 232.5 d |
| HD 46966 | | | | 46966 | 31567 | 06$^h$ 36$^m$ 25.89$^s$ | +06° 04′ 59.5″ | 6.87 | | | O8V | variable star, ΔV = 0.006$^m$ |
| V Mon | | | V | 44639 | 30326 | 06$^h$ 22$^m$ 43.50$^s$ | −02° 11′ 42.0″ | 6.87 | | 2194 | M6e | Mira variable, V$_{max}$ = 6$^m$, V$_{min}$ = 13.9$^m$, P = 340.5 d |
| V644 Mon | | | V644 | 51480 | 33436 | 06$^h$ 57$^m$ 09.38$^s$ | −10° 49′ 28.1″ | 6.93 | | 4900 | Ape | γ Cas variable, V$_{max}$ = 6.88$^m$, V$_{min}$ = 6.98$^m$ |
| HD 53367 | | | V750 | 53367 | 34116 | 07$^h$ 04$^m$ 25.53$^s$ | −10° 27′ 15.7″ | 6.96 | | 932 | B0IV:e | γ Cas variable, V$_{max}$ = 6.92$^m$, V$_{min}$ = 7.22$^m$ |
| Gliese 282 A | | | V869 | 61606 | 37349 | 07$^h$ 39$^m$ 59.33$^s$ | −03° 35′ 51.0″ | 7.18 | | 46.33 | K2V | component of the Gliese 282 system; BY Dra variable, ΔV = 0.02$^m$ |
| V505 Mon | | | V505 | 48914 | 32397 | 06$^h$ 45$^m$ 49.98$^s$ | +02° 29′ 57.4″ | 7.22 | | 2170 | B5Ib | β Lyr variable, V$_{max}$ = 7.15$^m$, V$_{min}$ = 7.65$^m$, P = 53.78 d |
| V614 Mon | | | V614 | 52432 | 33794 | 07$^h$ 01$^m$ 01.95$^s$ | −03° 15′ 09.1″ | 7.27 | | 1550 | C... | semiregular variable, V$_{max}$ = 7.01$^m$, V$_{min}$ = 7.36$^m$, P = 60 d |
| HD 46223 | | | | 46223 | 31149 | 06$^h$ 32$^m$ 09.31$^s$ | +04° 49′ 24.7″ | 7.28 | | 5200 | O5e | in NGC 2244; variable star, ΔV = 0.008$^m$ |
| HD 46149 | | | | 46149 | 31128 | 06$^h$ 31$^m$ 52.53$^s$ | +05° 01′ 59.2″ | 7.61 | | 5200 | O8.5V+B | in NGC 2244; spectroscopic binary; rotating and pulsating variable |
| HD 44219 | | | | 44219 | 30114 | 06$^h$ 20$^m$ 14.32$^s$ | −10° 43′ 30.0″ | 7.70 | 4.19 | 164 | G5 | has a planet (b) |
| HD 46375 | | | | 46375 | 31246 | 06$^h$ 33$^m$ 12.62$^s$ | +05° 27′ 46.5″ | 7.84 | 5.22 | 109 | K1V | has a planet (b) |
| HD 59435 | | | V827 | 59435 | 36419 | 07$^h$ 29$^m$ 35.45$^s$ | −09° 15′ 33.3″ | 7.97 | | 1210 | A5p | α$^2$ CVn variable, V$_{max}$ = 7.97$^m$, V$_{min}$ = 7.99$^m$, P = 3.59 d |
| HD 45583 | | | V682 | 45583 | 30789 | 06$^h$ 28$^m$ 10.76$^s$ | −04° 53′ 56.5″ | 7.97 | | 962 | B9 | α$^2$ CVn variable |
| HD 46380 | | | V728 | 46380 | 31199 | 06$^h$ 32$^m$ 43.23$^s$ | −07° 30′ 32.3″ | 8.00 | | 1480 | B2Vne | Be star |
| HD 45652 | | | | 45652 | 30905 | 06$^h$ 29$^m$ 13.19$^s$ | +10° 56′ 02.0″ | 8.13 | 5.34 | 118 | G8-K0 | Lusitânia, has a planet (b) |
| HD 46202 | | | | 46202 | | 06$^h$ 32$^m$ 10.47$^s$ | +04° 57′ 59.8″ | 8.18 | | 5200 | O9V | in NGC 2244; β Cep variable, ΔV = 0.01$^m$, P = 0.21 d |
| HD 66428 | | | | 66428 | 39417 | 08$^h$ 03$^m$ 28.67$^s$ | −01° 09′ 45.8″ | 8.25 | 4.55 | 180 | G5 | has a planet (b) |
| V753 Mon | | | V753 | 54975 | 34684 | 07$^h$ 10$^m$ 57.85$^s$ | −03° 52′ 43.2″ | 8.27 | | 605 | A8V | Algol variable, V$_{max}$ = 8.30$^m$, V$_{min}$ = 8.81$^m$, P = 0.68 d |
| V723 Mon | | | V723 | 45762 | 30891 | 06$^h$ 29$^m$ 04.66$^s$ | −05° 34′ 20.2″ | 8.28 | | 1700 | G0II | Long period variable, potential black hole binary |
| SV Mon | | | SV | 44320 | 30219 | 06$^h$ 21$^m$ 26.30$^s$ | +06° 28′ 12.6″ | 8.28 | | | G7II... | classical Cepheid, V$_{max}$ = 7.61$^m$, V$_{min}$ = 8.88$^m$, P = 15.23 d |
| HD 50064 | | | | 50064 | | 06$^h$ 51$^m$ 34.11$^s$ | +00° 17′ 50.4″ | 8.30 | | 9500 | B6:Ia | one of the most luminous stars known; α Cyg variable, V$_{max}$ = 8.02$^m$, V$_{min}$ = 8.41$^m$, P = 60 d |
| HD 47755 | | | V684 | 47755 | | 06$^h$ 40$^m$ 38.30$^s$ | +09° 47′ 15.8″ | 8.41 | | | B4 | Algol variable, V$_{max}$ = 8.32$^m$, V$_{min}$ = 8.41$^m$, P = 1.85 d |
| UX Mon | | | UX | 65607 | 39042 | 07$^h$ 59$^m$ 16.38$^s$ | −07° 30′ 17.9″ | 8.42 | | 5500 | A3 | Algol and δ Sct variable, V$_{max}$ = 8.22$^m$, V$_{min}$ = 9.16$^m$, P = 5.90 d |
| AU Mon | | | AU | 50846 | 33237 | 06$^h$ 54$^m$ 54.71$^s$ | −01° 22′ 32.8″ | 8.43 | | | B5IV + F8-G0III-II | double periodic or Algol variable, V$_{max}$ = 8.20$^m$, V$_{min}$ = 9.16$^m$, P = 11.11 d |
| HD 47732 | | | V641 | 47732 | 31939 | 06$^h$ 40$^m$ 28.59$^s$ | +09° 49′ 04.3″ | 8.46 | | 2190 | B3Vnn... | rotating ellipsoidal variable, ΔV = 0.07$^m$, P = 1.32 d |
| V578 Mon | | | V578 | 259135 | | 06$^h$ 32$^m$ 00.61$^s$ | +04° 52′ 40.9″ | 8.55 | | | B1:V:n | Algol variable, V$_{max}$ = 8.54$^m$, V$_{min}$ = 8.57$^m$, P = 2.41 d |
| HD 259431 | | | V700 | 259431 | 31235 | 06$^h$ 33$^m$ 05.19$^s$ | +10° 19′ 20.0″ | 8.72 | | 564 | B6ep | Orion variable, V$_{max}$ = 8.62$^m$, V$_{min}$ = 8.91$^m$ |
| AR Mon | | | AR | 57364 | 35600 | 07$^h$ 20$^m$ 48.45$^s$ | −05° 15′ 35.8″ | 8.79 | | 962 | K0II | RS CVn variable, V$_{max}$ = 8.62$^m$, V$_{min}$ = 9.47$^m$, P = 21.21 d |
| Gliese 282 B | | | | 61606B | | 07$^h$ 40$^m$ 02.88$^s$ | −03° 36′ 13.4″ | 8.93 | | 46.33 | K7V + | component of the Gliese 282 system |
| HD 44179 | | | V777 | 44179 | 30089 | 06$^h$ 19$^m$ 58.22$^s$ | −10° 38′ 14.7″ | 8.94 | | 1245 | B8V | central star of Red Rectangle Nebula; re-radiating binary system, V$_{max}$ = 8.78$^m$, V$_{min}$ = 8.94$^m$, P = 320 d |
| HD 49330 | | | V739 | 49330 | 32586 | 06$^h$ 47$^m$ 57.27$^s$ | +00° 46′ 34.0″ | 8.95 | | 1460 | B0.5IVe | γ Cas variable, V$_{max}$ = 8.72$^m$, V$_{min}$ = 9.02$^m$ |
| HD 50169 | | | | 50169 | 32965 | 06$^h$ 51$^m$ 59.23$^s$ | −01° 38′ 40.4″ | 8.99 | 1.69 | 1489 | A4p | Brewer's Star |
| FU Mon | | | FU | 44544 | 30301 | 06$^h$ 22$^m$ 23.85$^s$ | +03° 25′ 27.9″ | 9.06 | | 2490 | S6.5/7.5 | semiregular variable |
| TU Mon | | | TU | | 38523 | 07$^h$ 53$^m$ 19.75$^s$ | −03° 02′ 31.1″ | 9.24 | | 1960 | B5V + F3 | Algol variable |
| RW Mon | | | RW | 259986 | 31383 | 06$^h$ 34$^m$ 45.89$^s$ | +08° 49′ 32.18″ | 9.32 | | 738 | B8V + G5IV | Algol variable, V$_{max}$ = 9.26$^m$, V$_{min}$ = 11.51$^m$, P = 1.91 d |
| VV Mon | | | VV | | 34003 | 07$^h$ 03$^m$ 18.29$^s$ | −05° 44′ 15.5″ | 9.40 | | 434 | G0 | RS CVn variable, V$_{max}$ = 9.4$^m$, V$_{min}$ = 9.95$^m$, P = 6.05 d |
| BX Mon | | | BX | | | 07$^h$ 25$^m$ 22.78$^s$ | −03° 35′ 15.8″ | 9.50 | | | M5IIIpe | Z And variable, V$_{max}$ = 9.5$^m$, V$_{min}$ = 12.5$^m$, P = 1259 d |
| PZ Mon | | | PZ | 289114 | 32621 | 06$^h$ 48$^m$ 21.07$^s$ | +01° 13′ 08.3″ | 9.60 | | 2080 | K2Ve | irregular variable |
| V694 Mon | | | V694 | | | 07$^h$ 25$^m$ 51.29$^s$ | −07° 44′ 08.1″ | 9.70 | | 1550 | C... | Z And variable, V$_{max}$ = 9.2$^m$, V$_{min}$ = 11.4$^m$, P = 1931 d |
| AO Mon | | | AO | 53883 | 34299 | 07$^h$ 06$^m$ 36.30$^s$ | −04° 37′ 24.5″ | 9.72 | | | B3 + B5 | Algol and δ Sct variable, V$_{max}$ = 9.6$^m$, V$_{min}$ = 10.23$^m$, P = 1.88 d |
| V588 Mon | | | V588 | 261331 | | 06$^h$ 39$^m$ 05.90$^s$ | +09° 41′ 03.4″ | 9.75 | | | A7III/IV | δ Sct variable, V$_{max}$ = 9.66$^m$, V$_{min}$ = 9.72$^m$, P = 0.11 d |
| V372 Mon | | | V372 | | | 06$^h$ 41$^m$ 26.13$^s$ | −04° 35′ 45.8″ | 9.81 | | | SC7/7.5 | semiregular variable |
| CV Mon | | | CV | | 31624 | 06$^h$ 37$^m$ 04.84$^s$ | +03° 03′ 50.2″ | 9.90 | | | | in C0634+031; classical Cepheid, V$_{max}$ = 9.9$^m$, V$_{min}$ = 10.7$^m$, P = 5.38 d |
| G 112-29 | | | | | 36985 | 07$^h$ 36$^m$ 07.08$^s$ | −03° 06′ 38.8″ | 9.99 | | 46.21 | M: | component of the Gliese 282 system; rotating variable, V$_{max}$ = 0.19$^m$, V$_{min}$ = 12.16$^m$ |
| HD 50281B | | | | 50281B | | 06$^h$ 52$^m$ 18.05$^s$ | −05° 11′ 24.2″ | 10.05 | | | M2 | component of the HD 50281 system |
| V589 Mon | | | V589 | 261446 | | 06$^h$ 39$^m$ 28.46$^s$ | +09° 42′ 04.1″ | 10.27 | | | F2III | δ Sct variable, ΔV = 0.05$^m$, P = 0.12 d |
| BE Mon | | | BE | | 31905 | 06$^h$ 40$^m$ 05.58$^s$ | +07° 36′ 21.0″ | 10.5 | | | G5 | classical Cepheid, V$_{max}$ = 10.19$^m$, V$_{min}$ = 10.88$^m$, P = 2.71 d |
| RU Mon | | | RU | | 33163 | 06$^h$ 54$^m$ 12.31$^s$ | −07° 35′ 45.0″ | 10.51 | | | B9pv + B7V + B7.2V | Algol variable, V$_{max}$ = 10.33$^m$, V$_{min}$ = 11.18$^m$, P = 3.58 d |
| CL Mon | | | CL | | | 06$^h$ 55$^m$ 36.70$^s$ | +06° 22′ 43.3″ | 11.00 | | | C... | Mira variable, V$_{max}$ = 8.1$^m$, V$_{min}$ = 13.0$^m$, P = 493 d |
| Ross 614 | | | V577 | | 30920 | 06$^h$ 29$^m$ 23.40$^s$ | −02° 48′ 50.3″ | 11.08 | 13.01 | 13.4 | M4.5V + M8V | binary star; one component is a flare star |
| DD Mon | | | DD | 292319 | | 06$^h$ 45$^m$ 57.83$^s$ | −00° 07′ 31.9″ | | | | G0 | Algol variable |
| A0620-00 | | | V616 | | | 06$^h$ 22$^m$ 44.50$^s$ | −00° 20′ 44.7″ | 11.2 | | | K3V-K7V | X-ray nova and rotating ellipsoidal variable, V$_{max}$ = 11.0$^m$, V$_{min}$ = 18.3$^m$, P = 0.32 d |
| CS Mon | | | CS | | | 06$^h$ 32$^m$ 10.94$^s$ | +06° 39′ 11.0″ | 11.25 | | | | classical Cepheid, V$_{max}$ = 10.71$^m$, V$_{min}$ = 11.3$^m$, P = 6.73 d |
| COROT-7 | | | | | | 06$^h$ 43$^m$ 49.47$^s$ | −01° 03′ 46.9″ | 11.73 | 5.85 | 489 | K0V | has two planets (b & c) and one unconfirmed planet (d) |
| R Mon | | | R | | | 06$^h$ 39$^m$ 09.95$^s$ | +08° 44′ 10.8″ | 11.85 | | | B0 | in NGC 2261; Orion variable |
| BN Mon | | | BN | | | 06$^h$ 21$^m$ 58.00$^s$ | +07° 20′ 57.7″ | 12.70 | | | Nv... | semiregular variable |
| V396 Mon | | | V396 | | | 06$^h$ 38$^m$ 36.48$^s$ | +03° 36′ 17.1″ | | | | | W UMa variable |
| V590 Mon | | | V590 | | | 06$^h$ 40$^m$ 44.64$^s$ | +09° 48′ 02.1″ | 12.88 | | | B7 | Orion variable |
| COROT-4 | | | | | | 06$^h$ 48$^m$ 46.70$^s$ | −00° 40′ 22.0″ | 13.45 | | | F0V | has a transiting planet (b) |
| COROT-1 | | | | | | 06$^h$ 48$^m$ 19.17$^s$ | −03° 06′ 07.8″ | 13.6 | 5.2 | 1560 | G0V | first transiting planet by COROT mission (b) |
| VY Mon | | | VY | | | 06$^h$ 31$^m$ 06.92$^s$ | +10° 26′ 05.0″ | 13.70 | | | B8 | UX Ori star |
| COROT-5 | | | | | | 06$^h$ 45$^m$ 06.54$^s$ | +00° 48′ 54.9″ | 14 | 6 | 1300 | F9V | has a transiting planet (b) |
| COROT-20 | | | | | | 06$^h$ 30$^m$ 53$^s$ | +00° 13′ 37″ | 14.66 | | 4012 | G2V | has a transiting planet (b) |
| COROT-19 | | | | | | 06$^h$ 28$^m$ 08$^s$ | −00° 01′ 01″ | 14.78 | | 2609 | F9V | has a transiting planet (b) |
| COROT-18 | | | | | | 06$^h$ 32$^m$ 41$^s$ | −00° 01′ 54″ | 14.99 | | 2838 | G9 | has a transiting planet (b) |
| COROT-13 | | | | | | 06$^h$ 50$^m$ 53.07$^s$ | −05° 05′ 11.1″ | 15.04 | 4.45 | 4270 | G0V | has a transiting planet (b) |
| BT Mon | | | BT | | | 06$^h$ 43$^m$ 47.24$^s$ | −02° 01′ 13.9″ | 15.4 | | | G5V | nova and Algol variable, V$_{max}$ = 4.5$^m$, V$_{min}$ = 16.4$^m$, P = 0.33 d |
| COROT-12 | | | | | | 06$^h$ 43$^m$ 03.76$^s$ | −01° 17′ 47.1″ | 15.52 | 5.21 | 3760 | G2V | has a transiting planet (b) |
| V838 Mon | | | V838 | | | 07$^h$ 04$^m$ 04.85$^s$ | −03° 50′ 51.1″ | 15.74 | | 20000 | M6I/III + B3V | luminous red nova, V$_{max}$ = 6.7$^m$, V$_{min}$ = 16.05$^m$ |
| COROT-14 | | | | | | 06$^h$ 53$^m$ 41.80$^s$ | −05° 32′ 09.7″ | 16.03 | 5.40 | 4360 | F9V | has a transiting planet (b) |
| CW Mon | | | CW | | | 06$^h$ 36$^m$ 54.58$^s$ | +00° 02′ 17.3″ | 17.2 | | 5500 | A3 | SS Cyg variable, V$_{max}$ = 11.9$^m$, V$_{min}$ = 17.2$^m$, P = 0.18 d |
| Scholz's Star | | | | | | 07$^h$ 20$^m$ 03.25$^s$ | −08° 46′ 49.9″ | 18.3 | 19.4 | 19.65 | M9.5+T5C | Binary star |
| AFGL 961 | | | | | | 06$^h$ 34$^m$ 37.63$^s$ | +04° 12′ 42.8″ | | | | K3V-K7V | young stellar object |
| Monoceros R2 IRS 3 | | | | | | 06$^h$ 47$^m$ 47.8$^s$ | −06° 22′ 55″ | | | | | young stellar object |
| NGC 2264 IRS 1 | | | | | | 06$^h$ 41$^m$ 10.06$^s$ | +09° 29′ 35.8″ | | | | B2 | in NGC 2264; young stellar object |
| UGPS J072227.51-054031.2 | | | | | | 07$^h$ 22$^m$ 27.87$^s$ | −05° 40′ 31.1″ | | | 13 | T9 | brown dwarf |