# قائمة النجوم في كوكبة ذات الكرسي

قائمة النجوم في كوكبة ذات الكرسي (بالإنجليزية: List of stars in Cassiopeia)‏
| الاسم | تسمية باير | تسمية فلامستيد | تصنيف النجوم المتغيرة | كتالوج هنري درابر | كتالوج هيباركوس | مطلع مستقيم | الميل | القدر الظاهري | قدر مطلق | البعد. سنة ضوئية | تصنيف نجمي | الاسم التقليدي+ ملاحظات |
| ? Cas | ? | 27 | | 5394 | 4427 | 00 56 42.50 | +60° 43′ 00.3″ | 2.15 | ?4.22 | 613 | B0IV:evar | Tsih, Navi; prototype نجم قذيفي, V$_{max}$ = 1.6$^m$, V$_{min}$ = 3.0$^m$ |
| صدر ذات الكرسي | ? | 18 | | 3712 | 3179 | 00 40 30.39 | +56° 32′ 14.7″ | 2.24 | ?1.99 | 228 | K0II-IIIvar | Schedar |
| الكف الخصيب | ? | 11 | | 432 | 746 | 00 09 10.09 | +59° 09′ 00.8″ | 2.28 | 1.17 | 54 | F2III-IV | Caph; نجوم -دلتا- الدرع, V$_{max}$ = 2.25$^m$, V$_{min}$ = 2.29$^m$, P = 0.10 d |
| الركبة | ? | 37 | | 8538 | 6686 | 01 25 48.60 | +60° 14′ 07.5″ | 2.68 | 0.26 | 99 | A5Vv SB | Ruchbah; Algol variable, V$_{max}$ = 2.68$^m$, V$_{min}$ = 2.76$^m$, P = 759 d |
| ? Cas | ? | 45 | | 11415 | 8886 | 01 54 23.68 | +63° 40′ 12.5″ | 3.35 | ?2.31 | 442 | B2pvar | Segin; نجم متغير, ΔV = 0.002$^m$, P = 0.09 d |
| ظهر الناقة | ? | 24 | | 4614 | 3821 | 00 49 05.10 | +57° 48′ 59.6″ | 3.46 | 4.59 | 19 | G0V SB | RS CVn variable |
| ? Cas | ? | 17 | | 3360 | 2920 | 00 36 58.27 | +53° 53′ 49.0″ | 3.69 | ?2.62 | 597 | B2IV | suspected variable |
| 50 Cas | | 50 | | 12216 | 9598 | 02 03 26.19 | +72° 25′ 16.5″ | 3.95 | 0.47 | 162 | A2V | variable star, ΔV = 0.003$^m$, P = 0.80 d |
| ? Cas | ? | 15 | | 2905 | 2599 | 00 32 59.99 | +62° 55′ 54.4″ | 4.17 | ?6.34 | 4127 | B1Ia | متغير ألفا الدجاجة, V$_{max}$ = 4.12$^m$, V$_{min}$ = 4.21$^m$, P = 2.65 d |
| ? Cas | ? | 33 | | 6961 | 5542 | 01 11 05.93 | +55° 08′ 59.8″ | 4.34 | 1.22 | 137 | A7Vvar | Marfak; suspected variable |
| ? Cas | ? | | | 15089 | 11569 | 02 29 03.99 | +67° 24′ 08.6″ | 4.46 | 1.27 | 141 | A5p Sr | نجوم ألفا كلاب الصيد, V$_{max}$ = 4.45$^m$, V$_{min}$ = 4.53$^m$, P = 1.74 d |
| ? Cas | ? | 22 | | 4180 | 3504 | 00 44 43.50 | +48° 17′ 03.8″ | 4.48 | ?2.74 | 906 | B5III | نظام نجمي, ? Cas variable, V$_{max}$ = 4.31$^m$, V$_{min}$ = 4.62$^m$ |
| 48 Cas | A | 48 | | 12111 | 9480 | 02 01 57.55 | +70° 54′ 25.4″ | 4.49 | 1.72 | 117 | A3IV | quadruple star |
| رو ذات الكرسي | ? | 7 | | 224014 | 117863 | 23 54 23.04 | +57° 29′ 57.8″ | 4.51 | ?9.5 | 8500 | F8Ia0-M2I | عملاق فائق أصفر؛ semiregular variable, V$_{max}$ = 4.1$^m$, V$_{min}$ = 6.2$^m$, P = 320 d |
| ?$^2$ Cas | ?$^2$ | 28 | | 5395 | 4422 | 00 56 40.01 | +59° 10′ 52.2″ | 4.62 | 0.62 | 206 | G8III-IV | |
| ? Cas | ? | 39 | | 9408 | 7294 | 01 33 55.93 | +59° 13′ 55.5″ | 4.68 | 0.70 | 204 | K0III | |
| ? Cas | ? | 36 | | 8491 | 6692 | 01 25 55.90 | +68° 07′ 47.8″ | 4.72 | 0.86 | 193 | K0III | |
| ? Cas | ? | 14 | | 2772 | 2505 | 00 31 46.32 | +54° 31′ 20.4″ | 4.74 | ?0.44 | 354 | B8Vn | suspected variable |
| ? Cas | ? | 19 | | 3901 | 3300 | 00 42 03.88 | +50° 30′ 45.1″ | 4.80 | ?2.86 | 1109 | B2.5V | suspected variable |
| HR 244 | | | | 5015 | 4151 | 00 53 04.28 | +61° 07′ 24.8″ | 4.80 | 3.46 | 61 | F8V | نجم ثنائي |
| R Cas | | | R | 224490 | 118188 | 23 58 24.80 | +51° 23′ 19.0″ | 4.80 | | 410 | M6.5-9e | نجوم الأعجوبة, V$_{max}$ = 4.7$^m$, V$_{min}$ = 13.5$^m$, P = 430 d |
| ?$^1$ Cas | ?$^1$ | 26 | | 5234 | 4292 | 00 55 00.19 | +58° 58′ 22.1″ | 4.83 | ?0.65 | 406 | K2III | |
| 1 Cas | | 1 | | 218376 | 114104 | 23 06 36.81 | +59° 25′ 11.2″ | 4.84 | ?2.81 | 1105 | B0.5IV | |
| HD 19275 | | | | 19275 | 14862 | 03 11 56.24 | +74° 23′ 37.9″ | 4.85 | 1.37 | 162 | A2Vnn | |
| ? Cas | ? | 5 | | 223165 | 117301 | 23 47 03.39 | +58° 39′ 06.7″ | 4.88 | 1.26 | 173 | K1III | |
| ? Cas | ? | 8 | | 224572 | 118243 | 23 59 00.53 | +55° 45′ 17.8″ | 4.88 | ?3.47 | 1523 | B1V... | |
| AR Cas | | | AR | 221253 | 115990 | 23 30 01.92 | +58° 32′ 56.1″ | 4.89 | ?1.34 | 575 | B3IV | septuple star; Algol variable, V$_{max}$ = 4.82$^m$, V$_{min}$ = 4.96$^m$, P = 6.07 d |
| ? Cas | ? | 25 | | 4636 | 3801 | 00 48 49.99 | +50° 58′ 05.5″ | 4.90 | ?0.49 | 389 | B9III | |
| ? Cas | ? | 20 | | 4058 | 3414 | 00 43 28.09 | +47° 01′ 28.7″ | 4.95 | 1.31 | 174 | A5V | rotating ellipsoidal variable |
| ? Cas | ? | 34 | | 7927 | 6242 | 01 20 04.92 | +58° 13′ 53.8″ | 4.95 | ?4.32 | 2329 | F0Ia | foreground star appearing among إن جي سي 457؛ suspected variable |
| 4 Cas | | 4 | | 220652 | 115590 | 23 24 50.25 | +62° 16′ 58.2″ | 4.96 | ?1.91 | 771 | M1III | نجم متغير غير منتظم بطيئ, V$_{max}$ = 4.95$^m$, V$_{min}$ = 5.00$^m$ |
| ? Cas | ? | 46 | | 11529 | 9009 | 01 56 00.00 | +68° 41′ 07.0″ | 4.97 | ?1.69 | 701 | B8III | suspected variable |
| HD 3240 | | | | 3240 | 2854 | 00 36 08.29 | +54° 10′ 06.4″ | 5.08 | ?0.87 | 505 | B7III | |
| V509 Cas | | | V509 | 217476 | 113561 | 23 00 05.10 | +56° 56′ 43.4″ | 5.10 | ?6.77 | 7723 | F80 | yellow hypergiant; semiregular variable, V$_{max}$ = 4.75$^m$, V$_{min}$ = 5.5$^m$ |
| ? Cas | ? | 30 | | 6582 | 5336 | 01 08 12.92 | +54° 55′ 27.2″ | 5.17 | 5.78 | 25 | G5VIp/M5V | suspected variable |
| HD 15920 | | | | 15920 | 12273 | 02 38 02.09 | +72° 49′ 05.6″ | 5.17 | 0.69 | 256 | G8III | |
| 42 Cas | | 42 | | 10250 | 8016 | 01 42 55.73 | +70° 37′ 21.2″ | 5.18 | 0.51 | 281 | B9V | suspected Algol variable |
| 49 Cas | | 49 | | 12339 | 9763 | 02 05 31.58 | +76° 06′ 54.4″ | 5.22 | ?0.36 | 426 | G8III | |
| 47 Cas | | 47 | | 12230 | 9727 | 02 05 07.05 | +77° 16′ 53.2″ | 5.27 | 2.64 | 109 | F0Vn | |
| 40 Cas | | 40 | | 9774 | 7650 | 01 38 30.94 | +73° 02′ 24.3″ | 5.28 | ?0.40 | 447 | G8II-III | suspected variable |
| HD 11946 | | | | 11946 | 9312 | 01 59 37.99 | +64° 37′ 17.9″ | 5.29 | 0.81 | 257 | A0Vn | |
| 31 Cas | | 31 | | 6829 | 5518 | 01 10 39.27 | +68° 46′ 43.3″ | 5.32 | 0.38 | 318 | A0Vnn | |
| HD 4775 | | | | 4775 | 3951 | 00 50 43.57 | +64° 14′ 51.3″ | 5.35 | ?1.63 | 813 | A4V comp SB | variable star, ΔV = 0.008$^m$, P = 0.96 d |
| 12 Cas | | 12 | | 2011 | 1960 | 00 24 47.49 | +61° 49′ 51.8″ | 5.38 | ?1.47 | 763 | B9III | |
| HD 4222 | | | | 4222 | 3544 | 00 45 17.20 | +55° 13′ 17.1″ | 5.41 | 0.25 | 351 | A2Vs | |
| 23 Cas | | 23 | | 4382 | 3721 | 00 47 46.02 | +74° 50′ 51.3″ | 5.42 | ?1.54 | 803 | B8III | |
| 6 Cas | | 6 | V566 | 223385 | 117447 | 23 48 50.17 | +62° 12′ 52.3″ | 5.43 | ?8.06 | 6150 | A3Ia comp | ? Cyg variable, V$_{max}$ = 5.34$^m$, V$_{min}$ = 5.45$^m$, P = 37.26 d |
| HD 3474 | | | | 3574 | 3083 | 00 39 09.89 | +49° 21′ 16.5″ | 5.45 | ?2.60 | 1331 | K5III | |
| HD 9900 | | | | 9900 | 7617 | 01 38 07.56 | +57° 58′ 39.5″ | 5.55 | ?2.17 | 1140 | G5II | |
| HD 223173 | | | | 223173 | 117299 | 23 47 01.91 | +57° 27′ 05.0″ | 5.55 | ?3.00 | 1672 | K3II | slow irregular variable, V$_{max}$ = 5.51$^m$, V$_{min}$ = 5.54$^m$ |
| HD 5408 | | | | 5408 | 4440 | 00 56 46.94 | +60° 21′ 46.3″ | 5.56 | ?0.81 | 614 | B8V | |
| HD 6960 | | | | 6960 | 5566 | 01 11 25.52 | +64° 12′ 09.8″ | 5.56 | 0.06 | 410 | B9.5V | suspected نجم ثنائي |
| HD 220369 | | | | 220369 | 115395 | 23 22 32.52 | +60° 08′ 00.6″ | 5.56 | ?2.73 | 1482 | K3II | suspected variable |
| 10 Cas | | 10 | | 144 | 531 | 00 06 26.53 | +64° 11′ 46.2″ | 5.57 | ?1.82 | 982 | B9III | suspected variable |
| 32 Cas | | 32 | | 6972 | 5589 | 01 11 41.37 | +65° 01′ 08.0″ | 5.57 | 0.34 | 363 | B9IV | suspected variable |
| 43 Cas | | 43 | V557 | 10221 | 7965 | 01 42 20.44 | +68° 02′ 35.0″ | 5.57 | ?0.10 | 444 | A0p SiSr | ?$^2$ CVn variable, V$_{max}$ = 5.55$^m$, V$_{min}$ = 5.64$^m$, P = 3.18 d |
| HR 8832 | | | | 219134 | 114622 | 23 13 14.74 | +57° 10′ 03.5″ | 5.57 | 6.50 | 21 | K3Vvar | suspected variable; has 7 كوكب خارج المجموعة الشمسية |
| HR 9059 | | | V1022 | 224355 | 118077 | 23 57 08.49 | +55° 42′ 20.6″ | 5.57 | 1.45 | 218 | G8Ib | Algol variable, V$_{max}$ = 5.56$^m$, V$_{min}$ = 5.68$^m$, P = 12.16 d |
| HD 224893 | | | | 224893 | 124 | 00 01 37.02 | +61° 13′ 22.1″ | 5.58 | ?4.75 | 3791 | F0III | suspected variable |
| HD 1976 | | | V746 | 1976 | 1921 | 00 24 15.64 | +52° 01′ 11.7″ | 5.58 | ?2.54 | 1370 | B5IV | spectroscopic binary; slowly pulsating B star |
| HD 219623 | | | | 219623 | 114924 | 23 16 42.19 | +53° 12′ 50.6″ | 5.58 | 4.04 | 66 | F7V | |
| HD 2774 | | | | 2774 | 2497 | 00 31 41.21 | +52° 50′ 22.4″ | 5.59 | 0.18 | 393 | K2III | |
| 53 Cas | | 53 | | 12301 | 9573 | 02 03 00.19 | +64° 23′ 24.1″ | 5.59 | ?4.54 | 3468 | B8Ib | |
| HD 17948 | | | | 17948 | 13665 | 02 55 56.74 | +61° 31′ 15.8″ | 5.59 | 3.48 | 86 | F4V | |
| HR 511 | | | V987 | 10780 | 8362 | 01 47 44.06 | +63° 51′ 11.2″ | 5.63 | 5.64 | 33 | K0V | BY Draconis variable, ΔV = 0.05$^m$, P = 21.7 d |
| YZ Cas | | 21 | YZ | 4161 | 3572 | 00 45 39.11 | +74° 59′ 17.3″ | 5.64 | 0.89 | 290 | A2IV | triple system; Algol variable |
| 68 Cas | | 68 | | 4142 | 3478 | 00 44 26.23 | +47° 51′ 50.3″ | 5.66 | ?1.18 | 760 | B5V... | |
| 2 Cas | | 2 | | 218753 | 114365 | 23 09 44.14 | +59° 19′ 57.7″ | 5.68 | ?3.23 | 1976 | A5III | suspected variable |
| HD 9352 | | | | 9352 | 7251 | 01 33 25.71 | +58° 19′ 38.4″ | 5.69 | ?3.20 | 1952 | K0Ib+... | slow irregular variable, V$_{max}$ = 5.68$^m$, V$_{min}$ = 5.72$^m$ |
| HD 2054 | | | | 2054 | 1982 | 00 25 06.39 | +53° 02′ 48.4″ | 5.72 | ?0.33 | 528 | B9IV | suspected variable |
| HD 1239 | | | | 1239 | 1354 | 00 16 57.05 | +61° 31′ 59.5″ | 5.74 | ?0.73 | 642 | G8III | |
| HD 6676 | | | | 6676 | 5361 | 01 08 33.45 | +58° 15′ 48.5″ | 5.77 | ?0.43 | 567 | B8V | |
| HD 3283 | | | | 3283 | 2876 | 00 36 27.34 | +60° 19′ 34.4″ | 5.78 | ?4.29 | 3361 | A4III | |
| 44 Cas | | 44 | | 10425 | 8046 | 01 43 19.74 | +60° 33′ 04.9″ | 5.78 | ?1.46 | 913 | B8IIIn | |
| HD 225289 | | | V567 | 225289 | 418 | 00 05 06.13 | +61° 18′ 50.3″ | 5.80 | ?0.93 | 724 | B8MNp... | ?$^2$ CVn variable, V$_{max}$ = 5.71$^m$, V$_{min}$ = 5.81$^m$, P = 6.43 d |
| HD 16024 | | | | 16024 | 12239 | 02 37 36.01 | +65° 44′ 43.3″ | 5.80 | ?1.19 | 815 | K5III | |
| 38 Cas | | 38 | | 9021 | 7078 | 01 31 13.52 | +70° 15′ 53.2″ | 5.82 | 3.49 | 95 | F6V | |
| HD 3856 | | | | 3856 | 3299 | 00 42 03.44 | +66° 08′ 51.4″ | 5.83 | ?0.11 | 503 | G9III-IV | |
| HR 297 | | | | 6210 | 5021 | 01 04 19.55 | +61° 34′ 48.9″ | 5.83 | 1.31 | 261 | F6V | |
| HD 1279 | | | | 1279 | 1372 | 00 17 09.04 | +47° 56′ 50.7″ | 5.86 | ?1.47 | 953 | B7III | |
| HD 4440 | | | | 4440 | 3750 | 00 48 08.88 | +72° 40′ 28.0″ | 5.86 | 1.69 | 223 | K0IV | |
| HD 225009 | | | | 225009 | 207 | 00 02 36.08 | +66° 05′ 56.3″ | 5.87 | ?3.15 | 2076 | G8III | |
| V762 Cas | | | V762 | 7389 | 5926 | 01 16 11.90 | +71° 44′ 37.8″ | 5.87 | ?7.42 | 2760 | M3 | BY Draconis variable |
| HD 19065 | | | | 19065 | 14502 | 03 07 19.02 | +64° 03′ 27.4″ | 5.89 | ?0.27 | 557 | B9V | |
| 9 Cas | | 9 | | 225180 | 330 | 00 04 13.66 | +62° 17′ 15.6″ | 5.90 | ?4.35 | 3663 | A1III | suspected variable |
| HD 6130 | | | | 6130 | 4962 | 01 03 37.01 | +61° 04′ 29.4″ | 5.92 | ?2.41 | 1509 | F0II | |
| HD 2952 | | | | 2952 | 2611 | 00 33 10.32 | +54° 53′ 42.3″ | 5.93 | 0.62 | 376 | K0III | has a planet |
| HD 2626 | | | | 2626 | 2377 | 00 30 19.91 | +59° 58′ 39.2″ | 5.94 | ?0.77 | 718 | B9IIIn | |
| SU Cas | | | SU | 17463 | 13367 | 02 51 58.75 | +68° 53′ 18.7″ | 5.94 | ?2.24 | 1411 | F5:Ib-II | متغير قيفاوي كلاسيكي, V$_{max}$ = 5.7$^m$, V$_{min}$ = 6.18$^m$, P = 1.95 d |
| HD 16769 | | | | 16769 | 12821 | 02 44 49.67 | +67° 49′ 29.0″ | 5.95 | 0.47 | 406 | A5III | variable star |
| HD 5550 | | | | 5550 | 4572 | 00 58 31.00 | +66° 21′ 06.6″ | 5.97 | 0.66 | 376 | A0III | |
| HR 5 | | | V640 | 123 | 518 | 00 06 15.54 | +58° 26′ 12.1″ | 5.98 | 4.44 | 70 | G5V | eclipsing binary, ΔV = 0.066$^m$, P = 1.03 d |
| HD 6211 | | | | 6211 | 4998 | 01 04 02.39 | +52° 30′ 08.3″ | 5.99 | ?1.42 | 991 | K2 | |
| 52 Cas | | 52 | | 12279 | 9564 | 02 02 52.49 | +64° 54′ 05.4″ | 6.00 | 1.30 | 284 | A1Vn | |
| HD 11857 | | | | 11857 | 9220 | 01 58 33.22 | +61° 41′ 52.1″ | 6.02 | ?0.70 | 721 | B5III | suspected variable |
| V373 Cas | | | V373 | 224151 | 117957 | 23 55 33.84 | +57° 24′ 43.8″ | 6.03 | | | B0.5IIv SB | spectroscopic binary; eclipsing binary, V$_{max}$ = 5.9$^m$, V$_{min}$ = 6.3$^m$, P = 13.41 d |
| HD 4817 | | | | 4817 | 3988 | 00 51 16.39 | +61° 48′ 19.8″ | 6.04 | ?3.37 | 2489 | K5Ib | variable star, ΔV = 0.009$^m$, P = 4.32 d |
| 55 Cas | | 55 | | 13474 | 10438 | 02 14 29.10 | +66° 31′ 28.0″ | 6.05 | ?0.72 | 738 | B9V+... | suspected variable |
| AO Cas | | | AO | 1337 | 1415 | 00 17 43.07 | +51° 25′ 59.1″ | 6.11 | ?5.11 | 5719 | O9IIInn | متغير بيضاوي دوار, V$_{max}$ = 6.07$^m$, V$_{min}$ = 6.24$^m$, P = 3.52 d |
| HD 12173 | | | | 12173 | 9586 | 02 03 10.51 | +73° 51′ 02.0″ | 6.12 | 0.89 | 363 | A5III | |
| HD 9030 | | | | 9030 | 7050 | 01 30 52.01 | +66° 05′ 53.2″ | 6.15 | 1.46 | 282 | A2Vs | |
| HD 17958 | | | | 17958 | 13700 | 02 56 24.66 | +64° 19′ 56.8″ | 6.17 | ?1.80 | 1278 | K3Ibvar | |
| HD 224784 | | | | 224784 | 43 | 00 00 30.98 | +59° 33′ 35.1″ | 6.18 | 0.59 | 427 | G9III-IV | suspected variable |
| HD 2589 | | | | 2589 | 2422 | 00 30 54.20 | +77° 01′ 10.2″ | 6.18 | 3.20 | 128 | K0IV | |
| 13 Cas | | 13 | | 2729 | 2474 | 00 31 25.20 | +66° 31′ 10.7″ | 6.18 | ?0.53 | 716 | B6V | variable star, ΔV = 0.007$^m$, P = 1.08 d |
| HD 3924 | | | | 3924 | 3334 | 00 42 31.01 | +58° 45′ 12.4″ | 6.18 | ?1.29 | 1016 | B9.5III | |
| V773 Cas | | | V773 | 10543 | 8115 | 01 44 17.91 | +57° 32′ 12.0″ | 6.18 | 1.69 | 258 | A3V | Algol variable |
| HD 5343 | | | | 5343 | 4383 | 00 56 12.93 | +57° 59′ 47.7″ | 6.20 | 0.28 | 497 | K3III | |
| HD 224870 | | | | 224870 | 106 | 00 01 19.24 | +49° 58′ 53.7″ | 6.22 | ?0.51 | 724 | G7II-III | |
| HD 4881 | | | | 4881 | 4023 | 00 51 33.79 | +51° 34′ 17.2″ | 6.22 | ?1.51 | 1148 | B9.5V | |
| HD 225094 | | | V639 | 225094 | 274 | 00 03 25.72 | +63° 38′ 25.9″ | 6.24 | ?3.92 | 3505 | B3Ia | ? Cyg variable, V$_{max}$ = 6.19$^m$, V$_{min}$ = 6.28$^m$, P = 2.88 d |
| HD 217673 | | | | 217673 | 113684 | 23 01 30.72 | +57° 06′ 19.7″ | 6.24 | ?1.56 | 1181 | K2II | suspected variable |
| HD 222618 | | | | 222618 | 116912 | 23 41 54.56 | +57° 15′ 35.9″ | 6.24 | ?0.93 | 886 | G8III | |
| HD 10587 | | | | 10587 | 8148 | 01 44 46.15 | +57° 05′ 21.2″ | 6.25 | 0.07 | 560 | A2V | |
| HD 13222 | | | | 13222 | 10350 | 02 13 21.05 | +74° 01′ 40.1″ | 6.25 | 0.61 | 438 | G8III | |
| HD 21970 | | | | 21970 | 17056 | 03 39 25.10 | +75° 44′ 22.6″ | 6.25 | 0.65 | 429 | G9III-IV | |
| RZ Cas | | | RZ | 17138 | 13133 | 02 48 55.51 | +69° 38′ 03.1″ | 6.26 | 2.28 | 204 | A3V | Algol variable, V$_{max}$ = 6.18$^m$, V$_{min}$ = 7.72$^m$, P = 1.20 d |
| HD 222570 | | | | 222570 | 116876 | 23 41 26.80 | +49° 30′ 44.9″ | 6.26 | ?0.63 | 778 | A4V | |
| HD 5128 | | | | 5128 | 4212 | 00 53 47.53 | +52° 41′ 21.6″ | 6.27 | 1.61 | 278 | A5m | |
| HD 5273 | | | | 5273 | 4298 | 00 55 05.22 | +48° 40′ 42.8″ | 6.28 | ?0.68 | 803 | M2.5IIIa | variable star, ΔV = 0.012$^m$, P = 21.89 d |
| HD 6540 | | | | 6540 | 5251 | 01 07 09.44 | +53° 29′ 53.5″ | 6.31 | ?1.79 | 1358 | K0 | |
| HD 7732 | | | | 7732 | 6261 | 01 20 19.45 | +77° 34′ 13.7″ | 6.31 | 0.98 | 379 | G5III... | |
| 35 Cas | | 35 | | 8003 | 6312 | 01 21 05.19 | +64° 39′ 29.5″ | 6.33 | 2.01 | 238 | A2Vnn | |
| HD 10362 | | | | 10362 | 8020 | 01 42 58.32 | +61° 25′ 15.9″ | 6.33 | ?1.15 | 1022 | B7II | |
| HD 223386 | | | | 223386 | 117450 | 23 48 53.91 | +59° 58′ 44.2″ | 6.33 | 1.22 | 344 | A0V | |
| HD 8424 | | | | 8424 | 6685 | 01 25 46.30 | +70° 58′ 47.7″ | 6.34 | 0.35 | 514 | A0Vnn | |
| HD 10293 | | | | 10293 | 7963 | 01 42 17.69 | +58° 37′ 39.9″ | 6.35 | ?1.90 | 1455 | B8III | suspected variable |
| HD 8272 | | | | 8272 | 6486 | 01 23 21.27 | +58° 08′ 35.6″ | 6.36 | 2.56 | 188 | F4V | |
| HD 223421 | | | | 223421 | 117472 | 23 49 11.89 | +58° 57′ 47.6″ | 6.36 | 1.94 | 250 | F2IV | |
| HD 7925 | | | | 7925 | 6378 | 01 21 58.94 | +76° 14′ 20.0″ | 6.37 | 1.95 | 250 | F0IVn | |
| V805 Cas | | | V805 | 21179 | 16319 | 03 30 19.39 | +71° 51′ 50.0″ | 6.37 | ?0.73 | 856 | M2III | semiregular variable |
| HD 4818 | | | V526 | 4818 | 3965 | 00 50 57.27 | +51° 30′ 28.9″ | 6.38 | 2.26 | 217 | F2IV | ? Sct variable, ΔV = 0.03$^m$ |
| HD 4295 | | | | 4295 | 3641 | 00 46 38.23 | +69° 19′ 31.3″ | 6.39 | 3.35 | 132 | F3V | |
| HD 5357 | | | | 5357 | 4446 | 00 56 54.99 | +68° 46′ 32.7″ | 6.39 | 2.51 | 195 | F0m | |
| V465 Cas | | | V465 | 7733 | 6093 | 01 18 13.89 | +57° 48′ 11.4″ | 6.39 | ?0.75 | 874 | M5 | semiregular variable, V$_{max}$ = 6.1$^m$, V$_{min}$ = 7.2$^m$, P = 60 d |
| HD 220074 | | | | 220074 | 115218 | 23 20 14.37 | +61° 58′ 12.5″ | 6.39 | ?0.91 | 942 | K1V | suspected variable; has a planet |
| HD 5715 | | | | 5715 | 4709 | 01 00 30.87 | +70° 58′ 58.8″ | 6.40 | 1.21 | 355 | A4IV | |
| V761 Cas | | | V761 | 7157 | 5688 | 01 13 09.82 | +61° 42′ 22.3″ | 6.40 | ?0.11 | 652 | B9V | ?$^2$ CVn variable |
| HD 222682 | | | | 222682 | 116962 | 23 42 31.41 | +61° 40′ 45.8″ | 6.40 | 0.66 | 459 | K2III | |
| HD 371 | | | | 371 | 695 | 00 08 32.87 | +63° 12′ 14.6″ | 6.41 | ?1.91 | 1502 | G3II | |
| HD 2904 | | | | 2904 | 2628 | 00 33 19.20 | +70° 58′ 54.7″ | 6.41 | 0.36 | 528 | A0Vn | |
| HD 4362 | | | | 4362 | 3649 | 00 46 42.47 | +59° 34′ 28.3″ | 6.41 | | | G0Ib | |
| HD 6497 | | | | 6497 | 5240 | 01 07 00.07 | +56° 56′ 06.9″ | 6.41 | 1.47 | 318 | K2III... | |
| HD 218440 | | | | 218440 | 114163 | 23 07 10.45 | +59° 43′ 38.6″ | 6.41 | ?1.65 | 1336 | B2.5IV | |
| HD 220130 | | | | 220130 | 115245 | 23 20 34.54 | +62° 12′ 47.8″ | 6.41 | ?2.24 | 1753 | K2III | |
| HR 9017 | | | V650 | 223358 | 117430 | 23 48 39.03 | +64° 52′ 35.3″ | 6.41 | ?0.30 | 718 | A0sp... | ?$^2$ CVn variable, ΔV = 0.02$^m$ |
| HD 1142 | | | | 1142 | 1269 | 00 15 54.87 | +61° 00′ 00.7″ | 6.43 | 0.23 | 566 | G8III... | |
| HD 217944 | | | | 217944 | 113852 | 23 03 21.33 | +58° 33′ 50.0″ | 6.43 | 1.71 | 286 | G8IV | |
| HD 5459 | | | | 5459 | 4475 | 00 57 19.53 | +61° 25′ 19.0″ | 6.44 | 0.21 | 575 | G8IV | |
| HD 222748 | | | | 222748 | 116991 | 23 43 05.03 | +51° 56′ 21.6″ | 6.44 | 0.27 | 559 | K0 | |
| HD 1601 | | | | 1601 | 1639 | 00 20 30.92 | +48° 58′ 07.1″ | 6.46 | ?0.86 | 950 | G0 | |
| HD 17581 | | | | 17581 | 13347 | 02 51 45.92 | +58° 18′ 51.5″ | 6.46 | 1.75 | 285 | A1m | |
| HD 222932 | | | | 222932 | 117133 | 23 44 48.37 | +55° 47′ 58.9″ | 6.46 | 0.65 | 473 | G4III: | |
| 16 Cas | | 16 | | 3038 | 2707 | 00 34 24.89 | +66° 45′ 01.3″ | 6.47 | 0.28 | 565 | B9III | |
| V801 Cas | | | V801 | 19243 | 14626 | 03 08 54.18 | +62° 23′ 04.5″ | 6.47 | ?2.48 | 2012 | B1V:e | نجم-Be |
| HD 223552 | | | | 223552 | 117551 | 23 50 22.12 | +51° 37′ 18.1″ | 6.47 | 3.43 | 132 | F3V | |
| HD 224404 | | | | 224404 | 118116 | 23 57 33.52 | +60° 01′ 25.0″ | 6.47 | ?1.26 | 1144 | B9III-IV | |
| HD 5927 | | | | 5927 | 4786 | 01 01 27.04 | +49° 32′ 39.2″ | 6.48 | ?0.77 | 921 | G5 | |
| HD 6028 | | | | 6028 | 4844 | 01 02 18.47 | +51° 02′ 05.9″ | 6.48 | 0.04 | 632 | A3V | |
| HD 9811 | | | | 9811 | 7593 | 01 37 47.20 | +64° 44′ 21.7″ | 6.49 | ?3.30 | 2964 | A6Iab | |
| HR 8770 | | | V638 | 217833 | 113797 | 23 02 43.80 | +55° 14′ 11.0″ | 6.50 | | 723 | B9IIIwe... | ?$^2$ CVn variable |
| HD 19439 | | | | 19439 | 14791 | 03 11 00.80 | +64° 53′ 46.7″ | 6.50 | 2.03 | 256 | A4V | |
| V649 Cas | | | V649 | 219634 | 114904 | 23 16 27.05 | +61° 57′ 46.6″ | 6.53 | | 3500 | B0Vn | Algol variable, ΔV = 0.1$^m$, P = 2.39 d |
| 54 Cas | | 54 | | 12800 | 10031 | 02 09 07.69 | +71° 33′ 09.3″ | 6.57 | 4.39 | 89 | F8 | |
| V816 Cas | | | V816 | 222670 | 116948 | 23 42 20.95 | +64° 30′ 55.4″ | 6.58 | | 942 | M2III | slow irregular variable |
| V764 Cas | | | V764 | 7636 | 6027 | 01 17 26.69 | +57° 37′ 55.5″ | 6.61 | | 1900 | B2IIIne | Be star |
| V784 Cas | | | V784 | 13122 | 10141 | 02 10 25.5 | +59° 58′ 47.3″ | 6.64 | | 335 | F5II | ? Sct variable |
| V772 Cas | | | V772 | 10260 | 7939 | 01 42 02.91 | +61° 02′ 17.7″ | 6.69 | | 1220 | B8IIIsp... | Algol variable |
| V809 Cas | | | V809 | 219978 | 115141 | 23 19 23.77 | +62° 44′ 23.2″ | 6.74 | | 1960 | K4.5Ib | slow irregular variable |
| V779 Cas | | | V779 | 12013 | 9494 | 02 02 09.31 | +75° 30′ 07.8″ | 6.78 | | 626 | A0 | Algol variable |
| HD 11755 | | | | 11755 | 9242 | 01 58 50.0 | +73° 09′ 09″ | 6.87 | | 755 | G5 | has a planet (b) |
| TU Cas | | | TU | 2207 | 2085 | 00 26 19.45 | +51° 16′ 49.3″ | 6.88 | | | F3II... | double-mode Cepheid, V$_{max}$ = 6.88$^m$, V$_{min}$ = 8.18$^m$, P = 2.14 d |
| HD 223960 | | | V819 | 223960 | 117830 | 23 53 49.98 | +60° 51′ 12.2″ | 6.90 | | | A0.1Ia | ? Cyg variable |
| V Cas | | | V | 218997 | 114515 | 23 11 40.72 | +59° 41′ 59.0″ | 6.90 | | 1520 | M5-7.5e | Mira variable, V$_{max}$ = 6.9$^m$, V$_{min}$ = 13.4$^m$, P = 229 d |
| V486 Cas | | | V486 | 3950 | 3346 | 00 42 37.99 | +52° 20′ 13.7″ | 6.95 | | | B1III | eclipsing binary, ΔV = 0.04$^m$, P = 5.56 d |
| HD 14817 | | | V559 | 14817 | 11318 | 02 25 40.11 | +61° 32′ 58.8″ | 7.02 | | 695 | B8V | Algol variable, V$_{max}$ = 7.01$^m$, V$_{min}$ = 7.23$^m$, P = 1.58 d |
| V777 Cas | | | V777 | 11606 | 8980 | 01 55 42.85 | +59° 16′ 24.4″ | 7.02 | | 959 | B2Vne | Be star |
| HD 17505 | | | | 17505 | 13296 | 02 51 07.98 | +60° 25′ 03.9″ | 7.08 | | 2860 | O7V((f))+O9I | associated with a انحناء صدمي |
| CC Cas | | | CC | 19820 | 15063 | 03 14 05.33 | +59° 33′ 48.5″ | 7.08 | | 1860 | O8.5III | ? Lyr variable, V$_{max}$ = 7.06$^m$, V$_{min}$ = 7.3$^m$, P = 3.37 d |
| HD 698 | | | V742 | 698 | 940 | 00 11 37.15 | +58° 12′ 42.6″ | 7.08 | | 3500 | B7:Ib-IIe | Be star |
| V989 Cas | | | V989 | 13579 | 10531 | 02 15 42.56 | +67° 40′ 20.3″ | 7.13 | | 60.6 | K2V | BY Dra variable, ΔV = 0.03$^m$, P = 6.79 d |
| V636 Cas | | | V636 | 9250 | 7192 | 01 32 43.23 | +63° 35′ 37.7″ | 7.19 | | 1640 | G0Ib | classical Cepheid, V$_{max}$ = 7.09$^m$, V$_{min}$ = 7.26$^m$, P = 8.38 d |
| HD 7924 | | | | 7924 | 6379 | 01 21 59.12 | +76° 42′ 37.0″ | 7.19 | 6.06 | 55 | K0V | has three planets (HD 7924 b، c & d) |
| TV Cas | | | TV | 1486 | 1550 | 00 19 18.74 | +59° 08′ 20.6″ | 7.22 | | 516 | B9V | Algol variable, V$_{max}$ = 7.22$^m$, V$_{min}$ = 8.22$^m$, P = 1.81 d |
| V755 Cas | | | V755 | 3940 | 3367 | 00 42 50.06 | +64° 17′ 28.6″ | 7.29 | | 3700 | A1Ia | ? Cyg variable, V$_{max}$ = 7.25$^m$, V$_{min}$ = 7.31$^m$, P = 5.67 d |
| RV Cas | | | RV | 5016 | | 00 52 42.76 | +47° 24′ 56.1″ | 7.3 | | | M5-6.5Se | Mira variable, V$_{max}$ = 7.3$^m$, V$_{min}$ = 16.1$^m$, P = 332 d |
| HD 108 | | | | 108 | 505 | 00 06 03.39 | +63° 40′ 46.8″ | 7.40 | | 3800 | O4-8f?p | binary star; علم حركة النجوم؛ variable spectrum |
| HD 13908 | | | | 13908 | 10743 | 02 18 15.0 | +65° 35′ 40″ | 7.51 | | 232 | F8V | has two planets (b & c) |
| Gliese 83.3 | | | V598 | 12208 | 9481 | 02 01 59.06 | +61° 54′ 18.2″ | 7.52 | | 906 | K5III | slow irregular variable, V$_{max}$ = 7.38$^m$, V$_{min}$ = 7.54$^m$ |
| HD 221468 | | | V436 | 221568 | 116210 | 23 32 47.65 | +57° 54′ 20.1″ | 7.55 | | 709 | A0p | ?$^2$ CVn variable, V$_{max}$ = 7.55$^m$, V$_{min}$ = 7.62$^m$, P = 159 d |
| HD 19557 | | | V623 | 19557 | 14827 | 03 11 25.33 | +57° 54′ 11.2″ | 7.57 | | 1590 | C4,5J | slow irregular variable, V$_{max}$ = 7.34$^m$, V$_{min}$ = 7.96$^m$ |
| V487 Cas | | | V487 | 6474 | 5239 | 01 06 59.74 | +63° 46′ 23.4″ | 7.60 | | | G4Ia | نجم متغير شبة منتظم, V$_{max}$ = 7.44$^m$, V$_{min}$ = 7.74$^m$, P = 99.6 d |
| HD 16429 | | | V482 | 16429 | 12495 | 02 40 44.94 | +61° 16′ 56.1″ | 7.65 | | | O9.5III+F4V | triple star; ? Cep variable |
| WZ Cas | | | WZ | 224855 | 99 | 00 01 15.85 | +60° 21′ 19.0″ | 7.70 | | 2860 | C9,2JLi | semiregular variable, V$_{max}$ = 6.8$^m$, V$_{min}$ = 7.7$^m$, P = 186 d |
| HD 12288 | | | V540 | 12288 | 9604 | 02 03 30.51 | +69° 34′ 56.4″ | 7.74 | | 1010 | A2 | ?$^2$ CVn variable, V$_{max}$ = 7.73$^m$, V$_{min}$ = 7.75$^m$, P = 34.9 d |
| W Cas | | | W | 5235 | 4284 | 00 54 53.85 | +58° 33′ 49.1″ | 7.80 | | | C9,1e | Mira variable, V$_{max}$ = 7.8$^m$, V$_{min}$ = 12.5$^m$, P = 406 d |
| HD 15558 | | | | 15558 | 11832 | 02 32 42.54 | +61° 27′ 21.6″ | 7.87 | | | O4.5III | in سديم القلب؛ binary star; extremely luminous |
| S Cas | | | S | 7769 | | 01 19 41.99 | +72° 36′ 40.8″ | 7.9 | | | S3-5/4-8 | Mira variable, V$_{max}$ = 7.9$^m$, V$_{min}$ = 16.1$^m$, P = 612 d |
| U Cas | | | U | 4350 | | 00 46 21.37 | +48° 14′ 38.7″ | 8.0 | | | S4.5-6/3-5e | Mira variable, V$_{max}$ = 8$^m$, V$_{min}$ = 15.7$^m$, P = 277 d |
| HD 15570 | | | | 15570 | 11837 | 02 32 49.42 | +61° 22′ 42.1″ | 8.11 | | 2100 | O4If+ | in IC 1805 |
| V745 Cas | | | V745 | 1810 | 1805 | 00 22 53.32 | +62° 14′ 29.1″ | 8.11 | | | B0V+B1.5III | ? Lyr variable |
| HD 220147 | | | V812 | 220147 | 115267 | 23 20 48.92 | +62° 24′ 45.2″ | 8.12 | | 1060 | B9p | ?$^2$ CVn variable |
| HD 17156 | | | | 17156 | 13192 | 02 49 44.49 | +71° 45′ 11.6″ | 8.17 | 3.70 | 255 | G0IV | has a عبور فلكي |
| HD 240237 | | | | 240237 | 114840 | 23 15 42.22 | +58° 02′ 35.7″ | 8.17 | | | K2 | has a planet |
| HD 17520 | | | | 17520 | 13308 | 02 51 14.46 | +60° 23′ 09.8″ | 8.24 | | | O8V+O9:V | transitioned to a Be star in the 1980s |
| V641 Cas | | | V641 | | | 00 09 26.34 | +63° 57′ 14.1″ | 8.30 | | | M0 | semiregular variable |
| V368 Cas | | | V368 | 19644 | 14936 | 03 12 35.54 | +59° 55′ 10.9″ | 8.32 | | | B8II-III | Algol variable |
| HD 240210 | | | | 240210 | | 23 10 29.23 | +57° 01′ 46.0″ | 8.33 | 2.55 | 468 | K3III | has a planet |
| V605 Cas | | | V605 | 14242 | 10904 | 02 20 22.47 | +59° 40′ 16.9″ | 8.36 | | 1570 | M2Iab | slow irregular variable, V$_{max}$ = 8.22$^m$, V$_{min}$ = 8.48$^m$ |
| TW Cas | | | TW | 16907 | 12906 | 02 45 54.82 | +65° 43′ 35.1″ | 8.38 | | 849 | A0V | Algol variable, V$_{max}$ = 8.32$^m$, V$_{min}$ = 8.98$^m$, P = 1.43 d |
| HD 15629 | | | | 15629 | 11891 | 02 33 20.59 | +61° 31′ 18.2″ | 8.42 | | 1330 | O4.5V | in IC 1805 |
| HD 5797 | | | V551 | 5797 | 4717 | 01 00 33.43 | +60° 26′ 40.9″ | 8.47 | | 1490 | Am | ?$^2$ CVn variable, V$_{max}$ = 8.43$^m$, V$_{min}$ = 8.77$^m$, P = 69 d |
| Z Cas | | | Z | 222914 | | 23 44 31.59 | +56° 34′ 52.7″ | 8.5 | | | M7e | Mira variable, V$_{max}$ = 8.5$^m$, V$_{min}$ = 15.4$^m$, P = 496 d |
| DO Cas | | | DO | 16506 | 12543 | 02 41 24.16 | +60° 33′ 11.8″ | 8.54 | | 533 | A2II | ? Lyr variable, V$_{max}$ = 8.39$^m$, V$_{min}$ = 9.01$^m$, P = 0.68 d |
| HD 12098 | | | V988 | 12098 | | 02 00 40.18 | +58° 31′ 37.1″ | | | | F0 | نجم Ap سريع التذبذب |
| RW Cas | | | RW | | 7548 | 01 37 14.02 | +57° 45′ 33.2″ | 8.58 | | | G2 | classical Cepheid, V$_{max}$ = 8.62$^m$, V$_{min}$ = 9.67$^m$, P = 14.79 d |
| DL Cas | | | DL | 236429 | 2347 | 00 29 58.59 | +60° 12′ 43.1″ | 8.63 | | 1480 | G1Ib-II_Hdel-1 | in NGC 129؛ classical Cepheid, V$_{max}$ = 8.63$^m$, V$_{min}$ = 9.26$^m$, P = 8.00 d |
| RX Cas | | | RX | | 14542 | 03 05 45.75 | +67° 34′ 38.6″ | 8.64 | | | K1III+A5eIII | ? Lyr variable, V$_{max}$ = 8.64$^m$, V$_{min}$ = 9.49$^m$, P = 32.31 d |
| Y Cas | | | Y | 225082 | | 00 03 21.47 | +55° 40′ 51.8″ | 8.70 | | | M7.5e | Mira variable, V$_{max}$ = 8.7$^m$, V$_{min}$ = 15.3$^m$, P = 413 d |
| BD+60 2522 | | | | | | 23 20 44.52 | +61° 11′ 40.6″ | 8.7 | | 300 | O6.5III | source of nebula سديم الفقاعة |
| T Cas | | | T | 1845 | 1834 | 00 23 14.27 | +55° 47′ 33.2″ | 8.87 | | | M7-9e | Mira variable, V$_{max}$ = 6.9$^m$, V$_{min}$ = 13$^m$, P = 445 d |
| PZ Cas | | | PZ | | 117078 | 23 44 03.28 | +61° 47′ 22.2″ | 8.90 | | | M3Iab: | semiregular variable |
| BM Cas | | | BM | | 4279 | 00 54 45.95 | +64° 05′ 06.2″ | 8.91 | | 1850 | F0Ia | ? Lyr variable, V$_{max}$ = 8.78$^m$, V$_{min}$ = 9.31$^m$, P = 197 d |
| HD 219415 | | | | 219415 | | 23 14 54.0 | +56° 43′ 49″ | 8.94 | | | K0III | has a planet |
| SX Cas | | | SX | 232121 | 871 | 00 10 42.08 | +54° 53′ 29.4″ | 8.87 | | 771 | B5+K3III | Algol variable, V$_{max}$ = 8.96$^m$, V$_{min}$ = 9.83$^m$, P = 36.56 d |
| WW Cas | | | WW | | 7260 | 01 33 32.69 | +57° 45′ 05.4″ | 9.10 | | | C5,5 | slow irregular variable, V$_{max}$ = 9.1$^m$, V$_{min}$ = 11.7$^m$ |
| FM Cas | | | FM | 236349 | 1162 | 00 14 28.24 | +56° 15′ 10.6″ | 9.16 | | | F7.5Ib | classical Cepheid, V$_{max}$ = 8.82$^m$, V$_{min}$ = 9.47$^m$, P = 5.81 d |
| TZ Cas | | | TZ | | 117763 | 23 52 56.24 | +61° 00′ 08.4″ | 9.18 | | | M3Iab | slow irregular variable, V$_{max}$ = 8.86$^m$, V$_{min}$ = 10.5$^m$ |
| AZ Cas | | | AZ | | | 01 42 16.51 | +61° 25′ 16.3″ | 9.22 | | | M0Ib:ep+B | Algol variable, V$_{max}$ = 9.22$^m$, V$_{min}$ = 9.52$^m$, P = 3402 d |
| TX Cas | | | TX | | | 02 52 16.19 | +62° 46′ 57.5″ | 9.33 | | | B1V | ? Lyr variable, V$_{max}$ = 9.16$^m$, V$_{min}$ = 9.8$^m$, P = 2.93 d |
| X Cas | | | X | | 9057 | 01 56 38.09 | +59° 15′ 33.7″ | 9.45 | | 942 | C5,4e | Mira variable, V$_{max}$ = 9.45$^m$, V$_{min}$ = 13.2$^m$, P = 423 d |
| XX Cas | | | XX | | | 01 29 34.61 | +60° 58′ 04.7″ | 9.57 | | | B4Vn | Algol variable |
| SZ Cas | | | SZ | | 11420 | 02 27 13.77 | +59° 27′ 38.2″ | 9.60 | | 1210 | G5III | classical Cepheid, V$_{max}$ = 9.6$^m$, V$_{min}$ = 10.02$^m$, P = 13.63 d |
| SW Cas | | | SW | | 114160 | 23 07 10.08 | +58° 33′ 15.1″ | 9.74 | | 1520 | K0 | classical Cepheid, V$_{max}$ = 9.32$^m$, V$_{min}$ = 10.01$^m$, P = 5.44 d |
| UU Cas | | | UU | | 117576 | 23 50 39.52 | +60° 54′ 39.1″ | 9.74 | | | B1Iab: | ? Lyr variable |
| DD Cas | | | DD | | 118122 | 23 57 34.96 | +62° 43′ 05.7″ | 9.84 | | | F7 | classical Cepheid, V$_{max}$ = 9.56$^m$, V$_{min}$ = 10.18$^m$, P = 9.81 d |
| PV Cas | | | PV | 240208 | | 23 10 02.58 | +59° 12′ 06.1″ | 9.86 | | | B6V | Algol variable, V$_{max}$ = 9.71$^m$, V$_{min}$ = 10.36$^m$, P = 1.75 d |
| SY Cas | | | SY | | 1213 | 00 15 09.81 | +58° 25′ 27.4″ | 9.92 | | 1210 | F5 | classical Cepheid, V$_{max}$ = 9.4$^m$, V$_{min}$ = 10.24$^m$, P = 4.07 d |
| DN Cas | | | DN | | | 02 23 11.53 | +60° 49′ 50.1″ | 9.93 | | | O8Vv | Algol variable, V$_{max}$ = 9.81$^m$, V$_{min}$ = 10.24$^m$, P = 2.31 d |
| RY Cas | | | RY | | 117690 | 23 52 07.03 | +58° 44′ 30.2″ | 9.95 | | | F9Ib | classical Cepheid, V$_{max}$ = 9.38$^m$, V$_{min}$ = 10.39$^m$, P = 12.14 d |
| XY Cas | | | XY | 236542 | 3886 | 00 49 53.26 | +60° 07′ 38.6″ | 9.97 | | 1190 | F6Iab-b:... | classical Cepheid, V$_{max}$ = 9.61$^m$, V$_{min}$ = 10.26$^m$, P = 4.50 d |
| OX Cas | | | OX | | 5391 | 01 09 00.10 | +61° 28′ 14.8″ | 10.06 | | 1230 | B1V | Algol variable, V$_{max}$ = 9.9$^m$, V$_{min}$ = 10.35$^m$, P = 2.49 d |
| RS Cas | | | RS | | 116556 | 23 37 16.06 | +62° 25′ 44.4″ | 10.06 | | | F7-G1Ib | classical Cepheid, V$_{max}$ = 9.53$^m$, V$_{min}$ = 10.36$^m$, P = 6.39 d |
| QQ Cas | | | QQ | | | 23 45 36.75 | +59° 54′ 21.6″ | 10.20 | | | B2 | ? Lyr variable |
| V381 Cas | | | V381 | | | 00 32 51.61 | +49° 19′ 39.3″ | 10.22 | | | B | Algol variable |
| QX Cas | | | QX | | | 23 58 43.15 | +61° 09′ 39.5″ | 10.25 | | | B1V+B1V | Algol variable, V$_{max}$ = 10.19$^m$, V$_{min}$ = 10.7$^m$, P = 6.00 d |
| V547 Cas | | | V547 | | 2552 | 00 32 29.43 | +67° 14′ 08.4″ | 10.29 | | 32.8 | M2V+M3V | triple star; flare star |
| AQ Cas | | | AQ | | 6174 | 01 19 10.35 | +62° 23′ 48.4″ | 10.31 | | | B3 | Algol variable, V$_{max}$ = 10.06$^m$, V$_{min}$ = 11$^m$, P = 11.72 d |
| AB Cas | | | AB | | 12235 | 02 37 31.51 | +71° 18′ 16.3″ | 10.32 | | 888 | A3Vv+... | Algol and ? Sct variable, V$_{max}$ = 10.1$^m$, V$_{min}$ = 11.85$^m$, P = 1.37 d |
| V459 Cas | | | V459 | | | 01 11 29.92 | +61° 08′ 48.0″ | 10.36 | | | B9 | Algol variable |
| BY Cas | | | BY | | 8312 | 01 47 11.92 | +61° 25′ 21.0″ | 10.41 | | | F5 | classical Cepheid, V$_{max}$ = 10.06$^m$, V$_{min}$ = 10.58$^m$, P = 3.22 d |
| VX Cas | | | VX | | | 00 31 30.68 | +61° 58′ 51.0″ | 10.50 | | | A0Vep | هيربيغ أي/ نجم بي, V$_{max}$ = 10.5$^m$, V$_{min}$ = 13.3$^m$ |
| WR 1 | | | V863 | 4004 | 3415 | 00 43 28.40 | +64° 45′ 35.4″ | 10.54 | | | WN4-s | Algol variable, ΔV = 0.09$^m$ |
| MWC 419 | | | V594 | | 3401 | 00 43 18.26 | +61° 54′ 40.1″ | 10.60 | | 657 | B8eq | متغير جبار |
| CE Cas | | | CE | | | 23 58 09.31 | +61° 12′ 49.3″ | 10.63 | | 10800 | F9Ib+F8Ib | in NGC 7790؛ binary classical Cepheid, V$_{max}$ = 10.63$^m$, V$_{min}$ = 11.15$^m$, P = 5.14 d and V$_{max}$ = 10.62$^m$, V$_{min}$ = 11.30$^m$, P = 4.48 d |
| CD Cas | | | CD V405 | | 117154 | 23 45 02.63 | +63° 00′ 13.9″ | 10.64 | | 1230 | F6-G5 | classical Cepheid, V$_{max}$ = 10.37$^m$, V$_{min}$ = 11.15$^m$, P = 7.80 d |
| VW Cas | | | VW | | 5138 | 01 05 48.22 | +61° 45′ 17.8″ | 10.67 | | | K0 | classical Cepheid, V$_{max}$ = 10.36$^m$, V$_{min}$ = 11.07$^m$, P = 5.99 d |
| WR 3 | | | | 9974 | 7681 | 01 38 55.63 | +58° 09′ 22.7″ | 10.69 | | | WN3h-w | surrounded by a unique فقاعة الرياح النجمية |
| VV Cas | | | VV | | 8614 | 01 51 07.03 | +59° 53′ 17.5″ | 10.73 | | | F6 | classical Cepheid, V$_{max}$ = 10.26$^m$, V$_{min}$ = 11.2$^m$, P = 6.21 d |
| DF Cas | | | DF | | 12817 | 02 44 43.31 | +61° 27′ 52.9″ | 10.74 | | | F8 | classical Cepheid, V$_{max}$ = 10.53$^m$, V$_{min}$ = 11.13$^m$, P = 3.83 d |
| V364 Cas | | | V364 | | | 00 52 43.01 | +50° 28′ 10.2″ | 10.75 | | | A7 | Algol variable, V$_{max}$ = 10.53$^m$, V$_{min}$ = 11.22$^m$, P = 1.54 d |
| WY Cas | | | WY | | | 23 58 01.30 | +56° 29′ 13.5″ | 10.76 | | | S6-6.5/6-e | Mira variable |
| ZZ Cas | | | ZZ | | 2644 | 00 33 30.38 | +62° 30′ 40.2″ | 10.79 | | 1290 | B3 | ? Lyr variable |
| CH Cas | | | CH | | 115390 | 23 22 28.44 | +62° 45′ 25.7″ | 10.79 | | | F3Ibp | classical Cepheid, V$_{max}$ = 10.47$^m$, V$_{min}$ = 11.56$^m$, P = 15.09 d |
| CF Cas | | | CF | | 118174 | 23 58 17.98 | +61° 13′ 15.8″ | 10.80 | | 10800 | B3 | in NGC 7790; classical Cepheid, V$_{max}$ = 10.8$^m$, V$_{min}$ = 11.47$^m$, P = 4.88 d |
| BP Cas | | | BP | | 5846 | 01 15 01.09 | +65° 35′ 57.9″ | 10.80 | | | F6 | classical Cepheid, V$_{max}$ = 10.55$^m$, V$_{min}$ = 11.33$^m$, P = 6.27 d |
| LS I +61 303 | | | V615 | | 12469 | 02 40 31.67 | +61° 13′ 45.6″ | 10.8 | | | B0Ve | microquasar, V$_{max}$ = 10.4$^m$, V$_{min}$ = 11.1$^m$, P = 26.50 d |
| V523 Cas | | | V523 | | | 00 40 06.26 | +50° 14′ 15.5″ | 10.87 | | | K4V | W UMa variable, V$_{max}$ = 10.62$^m$, V$_{min}$ = 11.45$^m$, P = 0.23 d |
| CW Cas | | | CW | | | 00 45 52.69 | +63° 05′ 08.4″ | 11.08 | | 1340 | G8V | W UMa variable, V$_{max}$ = 11.02$^m$, V$_{min}$ = 11.62$^m$, P = 0.32 d |
| 2S 0114+650 | | | V662 | | 6081 | 01 18 02.70 | +65° 17′ 29.9″ | 11.09 | | | B1Iae | نباض الأشعة السينية, V$_{max}$ = 10.97$^m$, V$_{min}$ = 11.09$^m$, P = 11.60 d |
| IR Cas | | | IR | | | 23 06 52.37 | +54° 04′ 52.2″ | 11.14 | | | F4... | ? Lyr variable |
| IT Cas | | | IT | | | 23 42 01.40 | +51° 44′ 36.8″ | 11.23 | | | F6 | Algol variable |
| CG Cas | | | CG | | | 00 00 59.25 | +69° 57′ 32.2″ | 11.28 | | | F5 | classical Cepheid, V$_{max}$ = 10.89$^m$, V$_{min}$ = 11.73$^m$, P = 4.35 d |
| RX J0146.9+6121 | | | V831 | | | 01 47 00.21 | +61° 31′ 23.7″ | 11.34 | | | B1III-Ve | in NGC 663؛ X-ray pulsar, V$_{max}$ = 11.3$^m$, V$_{min}$ = 11.5$^m$ |
| IV Cas | | | IV | | | 23 49 31.53 | +53° 08′ 04.8″ | 11.34 | | | A2 | Algol and ? Sct variable |
| IX Cas | | | IX | | 390 | 00 04 50.82 | +50° 1405.5′ | 11.36 | | 637 | F7 | متغير العذراء W, V$_{max}$ = 11.19$^m$, V$_{min}$ = 11.77$^m$, P = 9.15 d |
| UZ Cas | | | UZ | | 5658 | 01 12 41.16 | +61° 12′ 48.1″ | 11.45 | | 1840 | G2 | classical Cepheid, V$_{max}$ = 10.93$^m$, V$_{min}$ = 11.73$^m$, P = 4.26 d |
| GP Cas | | | GP | | 12416 | 02 39 50.44 | +59° 35′ 51.3″ | 11.50 | | | M2Iab | slow irregular variable |
| MWC 1080 | | | V628 | | 114995 | 23 17 25.58 | +60° 50′ 43.4″ | 11.58 | | | B0eq | Orion variable, V$_{max}$ = 10.88$^m$, V$_{min}$ = 11.84$^m$ |
| CY Cas | | | CY | | 115925 | 23 29 12.77 | +63° 22′ 27.5″ | 11.67 | | | G1-2Ib | classical Cepheid, V$_{max}$ = 11.07$^m$, V$_{min}$ = 12.21$^m$, P = 14.38 d |
| UV Cas | | | UV | | | 23 02 14.66 | +59° 36′ 36.7″ | 11.80 | | | F0/5Ib | نجوم R الإكليل الشمالي |
| BS Cas | | | BS | | | 01 21 38.57 | +59° 10′ 27.1″ | 11.84 | | | A-F | W UMa variable, V$_{max}$ = 11.50$^m$, V$_{min}$ = 12.16$^m$, P = 0.44 d |
| Gliese 82 | | | V596 | | 9291 | 01 59 23.51 | +58° 31′ 16.1″ | 12.04 | | 39.9 | M4Ve | flare star |
| V627 Cas | | | V627 | | 113373 | 22 57 40.99 | +58° 09′ 12.5″ | 12.4 | | | M2eII-III | semiregular variable, V$_{max}$ = 12.4$^m$, V$_{min}$ = 13.24$^m$ |
| TY Cas | | | TY | | | 00 36 59.42 | +63° 08′ 01.7″ | | | | M6 | Mira variable |
| V592 Cas | | | V592 | | | 00 20 52.22 | +55° 42′ 16.3″ | 12.79 | | | OB | nova-like star, ΔV = 0.4$^m$, P = 0.12 d |
| HV Cas | | | HV | | | 01 11 03.48 | +53° 43′ 40.2″ | 12.9 | | | Ce | Mira variable |
| BH Cas | | | BH | | | 00 21 21.38 | +59° 09′ 05.4″ | 13 | | | B3 | W UMa variable, V$_{max}$ = 12.51$^m$, V$_{min}$ = 13.10$^m$, P = 0.41 d |
| IRAS 23304+6147 | | | | | | 23 32 44.79 | +62° 03′ 49.1″ | 13.1 | | | G2Ia | سديم كوكبي أولي, ΔV = 0.20$^m$, P = 85 d |
| HAT-P-44 | | | | | | 00 56 50.3 | +47° 00′ 52″ | 13.21 | | 1220 | | has two transiting planets |
| LkH? 198 | | | V633 | | | 00 11 25.83 | +58° 49′ 28.6″ | 13.79 | | | B9e | هيربيغ أي/ نجم بي؛ Orion variable |
| V664 Cas | | | V664 | | | 03 03 47.01 | +64° 54′ 35.7″ | 14.56 | | | | central star of HFG 1، re-radiating binary system |
| V425 Cas | | | V425 | | | 23 03 46.66 | +53° 17′ 14.9″ | | | | | منابع الأشعة السينية الفائقة الضعيفة |
| V709 Cas | | | V709 | | | 00 28 48.84 | +59° 17′ 22.0″ | | | | | متوسط القطبية (نجم متغير كارثي) |
| 4U 0115+634 | | | V635 | | | 01 18 31.90 | +63° 44′ 24.0″ | 15.19 | | | B0.2Ve | X-ray pulsar, V$_{max}$ = 14.5$^m$, V$_{min}$ = 16.3$^m$, P = 24.3 d |
| V376 Cas | | | V376 | | | 00 11 26.52 | +58° 50′ 03.7″ | | | | A3/F2e | Orion variable |
| IGR J00234+6141 | | | V1033 | | | 00 22 57.64 | +61° 41′ 07.6″ | 16.1 | | | | DQ Her variable, V$_{max}$ = 16.1$^m$, V$_{min}$ = 16.9$^m$, P = 0.17 d |
| V705 Cas | | | V705 | | | 23 41 47.19 | +57° 30′ 59.5″ | 16.4 | | | | مستعر, V$_{max}$ = 5.7$^m$, V$_{min}$ = 16.4$^m$ |
| Tycho G | | | | | | 00 25 19.9 | +64° 08′ 18″ | 17 | | | G2IV | former companion of progenitor of م أ 1572 |
| V723 Cas | | | V723 | | | 01 05 05.36 | +54° 00′ 40.3″ | 18.0 | | | A7 | nova, V$_{max}$ = 7.08$^m$, V$_{min}$ = <18.0$^m$ |
| RNO 1B | | | V710 | | | 00 36 46.30 | +63° 28′ 54.1″ | 18.6 | | | F8II | نجوم إف يو الجبار, V$_{max}$ = 18.6$^m$, V$_{min}$ = 21.6$^m$ |
| HT Cas | | | HT | | | 01 10 13.13 | +60° 04′ 35.4″ | 19.32 | | | M5.5e | مستعر قزم and eclipsing binary, V$_{max}$ = 12.6$^m$, V$_{min}$ = 19.32$^m$ |
| 4U 0142+61 | | | | | | 01 46 22.21 | +61° 45′ 03.8″ | 25.62 | | | | نجم مغناطيسي |
| IGR J00291+5934 | | | V1037 | | | 00 29 13.06 | +59° 34′ 19.0″ | | | | | X-ray pulsar with نباض ميلي ثانية |
| 1E 2259+586 | | | | | | 23 01 08.14 | +58° 52′ 44.5″ | | | | | نجم مغناطيسي |
| PSR B2319+60 | | | | | | 23 21 55.21 | +60° 24′ 30.7″ | | | | | نباض |
| PSR B2334+61 | | | | | | 23 37 05.78 | +61° 51′ 01.7″ | | | | | pulsar |
| 3 سي 58 | | | | | | 02 05 37.92 | +64° 49′ 42.8″ | | | | | central pulsar of 3 سي 58 |
| OH 127.8+0.0 | | | V669 | | | 01 33 51.21 | +62° 26′ 53.2″ | | | | M9III | Mira variable |
| W3 IRS 5 | | | | | | 02 25 40.54 | +62° 05′ 51.4″ | | | | B1 | نجم أولي؛ possibly similar to a proto-تجمع المعين |
| IRAS 00338+6312 | | | | | | 00 36 47.5 | +63° 29′ 02″ | | | | | protostar |

## اقرأ أيضا

* 3 ذات الكرسي