# List of stars in Vulpecula

This is the list of notable stars in the constellation Vulpecula, sorted by decreasing brightness.
| Name | B | F | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| α Vul | α | 6 | | 183439 | 95771 | 19$^h$ 28$^m$ 42.33$^s$ | +24° 39′ 53.7″ | 4.40 | −0.36 | 291 | M1III | Anser; suspected variable, V$_{max}$ = 4.39$^m$, V$_{min}$ = 4.46$^m$ |
| 23 Vul | | 23 | | 192806 | 99874 | 20$^h$ 15$^m$ 46.14$^s$ | +27° 48′ 51.1″ | 4.52 | −0.58 | 327 | K3- III Fe-1 | |
| 31 Vul | (r) | 31 | | 198809 | 103004 | 20$^h$ 52$^m$ 07.68$^s$ | +27° 05′ 49.0″ | 4.56 | 0.77 | 228 | G7IIIa Fe-1 Ba | |
| 13 Vul | | 13 | | 188260 | 97886 | 19$^h$ 53$^m$ 27.68$^s$ | +24° 04′ 46.3″ | 4.57 | −0.64 | 359 | B9.5III | |
| 15 Vul | | 15 | NT | 189849 | 98543 | 20$^h$ 01$^m$ 06.01$^s$ | +27° 45′ 12.8″ | 4.66 | 0.49 | 222 | A4III | α² CVn variable, V$_{max}$ = 4.62$^m$, V$_{min}$ = 4.67$^m$, P = 14 d |
| 1 Vul | | 1 | | 180554 | 94703 | 19$^h$ 16$^m$ 13.04$^s$ | +21° 23′ 25.6″ | 4.76 | −2.47 | 911 | B4IV | suspected variable, V$_{max}$ = 4.57$^m$, V$_{min}$ = 4.77$^m$ |
| HR 7739 | | | QR | 192685 | 99824 | 20$^h$ 15$^m$ 15.89$^s$ | +25° 35′ 31.1″ | 4.79 | −3.04 | 1199 | B3V | γ Cas variable, V$_{max}$ = 4.6$^m$, V$_{min}$ = 4.8$^m$ |
| 29 Vul | | 29 | | 196724 | 101867 | 20$^h$ 38$^m$ 31.29$^s$ | +21° 12′ 04.2″ | 4.81 | 0.73 | 213 | A0V | |
| 12 Vul | | 12 | V395 | 187811 | 97679 | 19$^h$ 51$^m$ 04.09$^s$ | +22° 36′ 36.3″ | 4.90 | −1.49 | 619 | B2.5V | Be star, V$_{max}$ = 4.78$^m$, V$_{min}$ = 4.97$^m$ |
| 30 Vul | | 30 | | 197752 | 102388 | 20$^h$ 44$^m$ 52.52$^s$ | +25° 16′ 15.8″ | 4.92 | −0.32 | 365 | K2III | |
| 9 Vul | | 9 | | 184606 | 96275 | 19$^h$ 34$^m$ 34.89$^s$ | +19° 46′ 24.2″ | 5.00 | −1.35 | 608 | B8IIIn | suspected variable, V$_{max}$ = 4.99$^m$, V$_{min}$ = 5.08$^m$ |
| 32 Vul | (q) | 32 | | 199169 | 103200 | 20$^h$ 54$^m$ 33.64$^s$ | +28° 03′ 27.5″ | 5.03 | −1.75 | 739 | K4III | suspected variable, V$_{max}$ = 4.99$^m$, V$_{min}$ = 5.06$^m$ |
| 28 Vul | | 28 | | 196740 | 101868 | 20$^h$ 38$^m$ 31.91$^s$ | +24° 06′ 57.5″ | 5.06 | −0.84 | 493 | B5IV | |
| 17 Vul | | 17 | | 190993 | 99080 | 20$^h$ 06$^m$ 53.40$^s$ | +23° 36′ 51.9″ | 5.08 | −0.80 | 488 | B3V | |
| 4 Vul | | 4 | | 182762 | 95498 | 19$^h$ 25$^m$ 28.54$^s$ | +19° 47′ 54.7″ | 5.14 | 0.84 | 237 | K0III | |
| 22 Vul | | 22 | QS | 192713 | 99853 | 20$^h$ 15$^m$ 30.24$^s$ | +23° 30′ 32.1″ | 5.15 | −5.44 | 4347 | G2Ib SB | Algol variable, ΔV = 0.12$^m$, P = 249.083 d |
| 3 Vul | | 3 | V377 | 182255 | 95260 | 19$^h$ 22$^m$ 50.88$^s$ | +26° 15′ 44.7″ | 5.18 | −0.24 | 402 | B6III | 53 Persei variable, ΔV = 0.03$^m$, P = 1.26239 d |
| 21 Vul | | 21 | NU | 192518 | 99738 | 20$^h$ 14$^m$ 14.52$^s$ | +28° 41′ 41.5″ | 5.19 | 0.18 | 327 | A7IVn | δ Sct variable |
| 16 Vul | | 16 | | 190004 | 98636 | 20$^h$ 02$^m$ 01.37$^s$ | +24° 56′ 16.3″ | 5.23 | 1.17 | 211 | F2III | |
| 24 Vul | | 24 | | 192944 | 99951 | 20$^h$ 16$^m$ 47.08$^s$ | +24° 40′ 16.1″ | 5.30 | −0.50 | 472 | G8III | |
| 33 Vul | | 33 | | 199697 | 103511 | 20$^h$ 58$^m$ 16.35$^s$ | +22° 19′ 33.3″ | 5.30 | −0.13 | 397 | K4III | |
| 35 Vul | | 35 | | 204414 | 105966 | 21$^h$ 27$^m$ 40.03$^s$ | +27° 36′ 30.8″ | 5.39 | 1.66 | 182 | A1V | |
| 2 Vul | | 2 | ES | 180968 | 94827 | 19$^h$ 17$^m$ 43.64$^s$ | +23° 01′ 32.0″ | 5.42 | −3.39 | 1918 | B0.5IV | β Cep variable, ΔV = 0.06$^m$, P = 0.6096 d |
| 10 Vul | | 10 | | 186486 | 97077 | 19$^h$ 43$^m$ 42.92$^s$ | +25° 46′ 18.7″ | 5.50 | 0.31 | 356 | G8III | |
| 25 Vul | | 25 | | 193911 | 100435 | 20$^h$ 22$^m$ 03.43$^s$ | +24° 26′ 46.0″ | 5.50 | −3.21 | 1801 | B8IIIn | suspected variable, V$_{max}$ = 5.51$^m$, V$_{min}$ = 5.54$^m$ |
| 19 Vul | | 19 | | 192004 | 99518 | 20$^h$ 11$^m$ 47.97$^s$ | +26° 48′ 32.5″ | 5.51 | −2.96 | 1614 | K3II-III | |
| 18 Vul | | 18 | | 191747 | 99404 | 20$^h$ 10$^m$ 33.52$^s$ | +26° 54′ 14.9″ | 5.53 | −0.04 | 420 | A3III | δ Sct variable, V$_{max}$ = 5.52$^m$, V$_{min}$ = 5.53$^m$ |
| HD 187982 | | | | 187982 | 97765 | 19$^h$ 52$^m$ 01.59$^s$ | +24° 59′ 31.8″ | 5.54 | −3.15 | 1781 | A1Iab | suspected variable, V$_{max}$ = 5.52$^m$, V$_{min}$ = 5.58$^m$ |
| HD 188485 | | | | 188485 | 97961 | 19$^h$ 54$^m$ 31.06$^s$ | +24° 19′ 09.8″ | 5.56 | −0.25 | 472 | A0III | variable star, ΔV = 0.005$^m$, P = 0.31928 d |
| 27 Vul | | 27 | | 196504 | 101716 | 20$^h$ 37$^m$ 04.66$^s$ | +26° 27′ 43.1″ | 5.59 | 0.73 | 305 | B9V | |
| 5 Vul | | 5 | | 182919 | 95560 | 19$^h$ 26$^m$ 13.24$^s$ | +20° 05′ 52.2″ | 5.60 | 1.47 | 218 | A0V | |
| T Vul | | | T | 198726 | 102949 | 20$^h$ 51$^m$ 28.24$^s$ | +28° 15′ 01.9″ | 5.66 | −2.89 | 1672 | F5Ib | classical Cepheid, V$_{max}$ = 5.41$^m$, V$_{min}$ = 6.09$^m$, P = 4.435462 d |
| HD 194577 | | | | 194577 | 100754 | 20$^h$ 25$^m$ 40.52$^s$ | +21° 24′ 34.8″ | 5.66 | −0.43 | 543 | G6III | suspected variable, ΔV = 0.04$^m$ |
| HD 203925 | | | | 203925 | 105703 | 21$^h$ 24$^m$ 33.97$^s$ | +26° 10′ 28.4″ | 5.67 | 1.53 | 220 | A8III | |
| 14 Vul | | 14 | | 189410 | 98375 | 19$^h$ 59$^m$ 10.58$^s$ | +23° 06′ 04.6″ | 5.68 | 2.26 | 158 | F0 | |
| HD 203803 | | | | 203803 | 105652 | 21$^h$ 23$^m$ 58.74$^s$ | +24° 16′ 26.7″ | 5.70 | 1.98 | 181 | F1IV | |
| HD 178187 | | | | 178187 | 93845 | 19$^h$ 06$^m$ 38.36$^s$ | +24° 15′ 02.7″ | 5.78 | 0.74 | 332 | A4III | |
| 8 Vul | | 8 | | 183491 | 95785 | 19$^h$ 28$^m$ 57.08$^s$ | +24° 46′ 07.3″ | 5.82 | −0.04 | 484 | K0III | suspected variable |
| HD 182955 | | | | 182955 | 95582 | 19$^h$ 26$^m$ 28.69$^s$ | +19° 53′ 29.8″ | 5.85 | 0.12 | 455 | M0III | slow irregular variable, ΔV = 0.01$^m$ |
| HD 189944 | | | | 189944 | 98609 | 20$^h$ 01$^m$ 44.71$^s$ | +24° 48′ 01.5″ | 5.88 | −0.69 | 672 | B4V | |
| HD 184010 | | | | 184010 | 96016 | 19$^h$ 31$^m$ 21.61$^s$ | +26° 37′ 01.6″ | 5.89 | 2.03 | 193 | K0III-IV | suspected variable |
| 20 Vul | | 20 | | 192044 | 99531 | 20$^h$ 12$^m$ 00.70$^s$ | +26° 28′ 43.8″ | 5.91 | −1.81 | 1140 | B7Ve... | variable star, V$_{max}$ = 5.87$^m$, V$_{min}$ = 5.92$^m$ |
| HD 196753 | | | | 196753 | 101870 | 20$^h$ 38$^m$ 34.99$^s$ | +23° 40′ 49.8″ | 5.91 | −3.00 | 1976 | K0II-III+.. | |
| HD 187193 | | | | 187193 | 97402 | 19$^h$ 47$^m$ 48.50$^s$ | +25° 23′ 02.8″ | 6.00 | 0.56 | 400 | K0II-III | |
| HD 179648 | | | | 179648 | 94382 | 19$^h$ 12$^m$ 36.72$^s$ | +21° 33′ 16.4″ | 6.02 | −1.43 | 1006 | A2Vn | |
| HD 196821 | | | | 196821 | 101919 | 20$^h$ 39$^m$ 10.63$^s$ | +21° 49′ 02.7″ | 6.08 | −1.19 | 926 | A0III | suspected variable |
| HD 201051 | | | | 201051 | 104172 | 21$^h$ 06$^m$ 23.45$^s$ | +26° 55′ 27.9″ | 6.13 | 0.99 | 348 | K0II-III | |
| 3 Cyg | | (3) | | 182807 | 95492 | 19$^h$ 25$^m$ 25.87$^s$ | +24° 54′ 51.5″ | 6.19 | 3.97 | 90 | F7V | |
| HD 203858 | | | | 203858 | 105660 | 21$^h$ 24$^m$ 07.42$^s$ | +25° 18′ 44.6″ | 6.20 | −0.17 | 612 | A2V | |
| HD 178476 | | | | 178476 | 93975 | 19$^h$ 08$^m$ 03.49$^s$ | +21° 41′ 55.5″ | 6.22 | 3.01 | 143 | F3V | |
| HD 191877 | | | | 191877 | 99479 | 20$^h$ 11$^m$ 21.02$^s$ | +21° 52′ 29.9″ | 6.24 | −8.55 | 6200 | B1Ib | |
| HD 193094 | | | | 193094 | 100018 | 20$^h$ 17$^m$ 31.54$^s$ | +29° 08′ 51.0″ | 6.24 | 0.98 | 367 | G9III | |
| PS Vul | | | PS | 186518 | 97091 | 19$^h$ 43$^m$ 55.97$^s$ | +27° 08′ 07.5″ | 6.28 | −4.35 | 4347 | B7V + G1:III | Algol variable, V$_{max}$ = 6.28$^m$, V$_{min}$ = 6.35$^m$, P = 3.8173 d |
| V387 Vul | | | V387 | 176541 | 93270 | 18$^h$ 59$^m$ 58.12$^s$ | +22° 48′ 52.2″ | 6.28 | −0.55 | 756 | M4III | semiregular variable |
| HD 203206 | | | | 203206 | 105344 | 21$^h$ 20$^m$ 14.07$^s$ | +22° 01′ 34.2″ | 6.29 | 0.20 | 539 | B6IV | suspected variable |
| HR 7556 | | | V379 | 187640 | 97572 | 19$^h$ 49$^m$ 54.72$^s$ | +28° 26′ 22.8″ | 6.29 | −2.13 | 1698 | B5V | rotating ellipsoidal variable, V$_{max}$ = 6.22$^m$, V$_{min}$ = 6.29$^m$ |
| HD 182761 | | | | 182761 | 95487 | 19$^h$ 25$^m$ 22.40$^s$ | +20° 16′ 18.4″ | 6.31 | 0.87 | 400 | A0V | |
| HD 184961 | | | | 184961 | 96417 | 19$^h$ 36$^m$ 08.35$^s$ | +22° 35′ 08.8″ | 6.33 | 0.11 | 571 | B9sp... | suspected variable |
| 7 Vul | | 7 | | 183537 | 95818 | 19$^h$ 29$^m$ 20.90$^s$ | +20° 16′ 47.2″ | 6.34 | −0.50 | 760 | B5Vn | variable star, ΔV = 0.009$^m$, P = 0.55923 d |
| HD 203886 | | | | 203886 | 105689 | 21$^h$ 24$^m$ 23.11$^s$ | +24° 31′ 42.3″ | 6.35 | 0.39 | 508 | K0III | |
| HD 195692 | | | | 195692 | 101300 | 20$^h$ 31$^m$ 58.19$^s$ | +25° 48′ 18.1″ | 6.37 | 1.82 | 264 | Am | |
| HD 182422 | | | | 182422 | 95340 | 19$^h$ 23$^m$ 46.93$^s$ | +20° 15′ 51.7″ | 6.40 | −1.30 | 1132 | B9.5V | |
| 26 Vul | | 26 | | 196362 | 101641 | 20$^h$ 36$^m$ 08.32$^s$ | +25° 52′ 57.4″ | 6.40 | −0.26 | 701 | A5III | |
| HD 186021 | | | | 186021 | 96856 | 19$^h$ 41$^m$ 14.65$^s$ | +22° 27′ 10.0″ | 6.43 | −1.80 | 1442 | K0Iab: | |
| HD 176971 | | | | 176971 | 93443 | 19$^h$ 01$^m$ 49.42$^s$ | +22° 15′ 51.8″ | 6.44 | 0.92 | 414 | A4V | |
| HD 190322 | | | | 190322 | 98772 | 20$^h$ 03$^m$ 38.81$^s$ | +22° 56′ 27.9″ | 6.45 | 0.46 | 513 | K2 | |
| HD 187614 | | | | 187614 | 97573 | 19$^h$ 49$^m$ 55.81$^s$ | +27° 05′ 06.6″ | 6.46 | 0.64 | 475 | G8III | |
| HD 189671 | | | | 189671 | 98458 | 20$^h$ 00$^m$ 15.36$^s$ | +26° 11′ 16.5″ | 6.49 | −1.79 | 1475 | G8II | |
| HD 196035 | | | | 196035 | 101505 | 20$^h$ 34$^m$ 09.98$^s$ | +20° 59′ 06.7″ | 6.49 | −1.79 | 1475 | B3IV | |
| HD 185436 | | | | 185436 | 96601 | 19$^h$ 38$^m$ 17.79$^s$ | +20° 47′ 00.5″ | 6.50 | 0.28 | 572 | K0III | |
| HD 190066 | | | | 190066 | 98661 | 20$^h$ 02$^m$ 22.11$^s$ | +22° 09′ 05.4″ | 6.50 | −3.75 | 3663 | B1Iab | |
| BW Vul | | | BW | 199140 | 103191 | 20$^h$ 54$^m$ 22.39$^s$ | +28° 31′ 19.2″ | 6.54 | −2.13 | 1772 | B2IIIvar | β Cep variable, V$_{max}$ = 6.44$^m$, V$_{min}$ = 6.68$^m$, P = 0.20104117 d |
| HR 7222 | | | LT | 177392 | 93603 | 19$^h$ 03$^m$ 42.48$^s$ | +21° 16′ 06.1″ | 6.62 | | 373 | F2III | δ Sct variable, V$_{max}$ = 6.52$^m$, V$_{min}$ = 6.62$^m$, P = 0.109 d |
| HD 192913 | | | MW | 192913 | 99927 | 20$^h$ 16$^m$ 27.20$^s$ | +27° 46′ 33.9″ | 6.64 | | 1610 | A0p | α$^2$ CVn variable, V$_{max}$ = 6.62$^m$, V$_{min}$ = 6.7$^m$, P = 16.846 d |
| SV Vul | | | SV | 187921 | 97717 | 19$^h$ 51$^m$ 03.91$^s$ | +27° 27′ 36.8″ | 6.74 | | 4100 | G2.5:Iab | classical Cepheid, V$_{max}$ = 6.72$^m$, V$_{min}$ = 7.79$^m$, P = 44.993 d |
| RS Vul | | | RS | 180939 | 94822 | 19$^h$ 17$^m$ 39.99$^s$ | +22° 26′ 28.4″ | 6.85 | | 939 | B5V+G0III-IV | Algol variable, V$_{max}$ = 6.79$^m$, V$_{min}$ = 7.83$^m$, P = 4.4776635 d |
| HIP 100963 | | | | 195034 | 100963 | 20$^h$ 28$^m$ 11.81$^s$ | +22° 07′ 44.4″ | 7.09 | | 92.04 | G5 | solar twin |
| U Vul | | | U | 185059 | 96458 | 19$^h$ 36$^m$ 37.73$^s$ | +20° 19′ 58.6″ | 7.15 | | 4900 | F5:Iabv | classical Cepheid, V$_{max}$ = 6.73$^m$, V$_{min}$ = 7.54$^m$, P = 7.990676 d |
| HD 190228 | | | | 190228 | 98714 | 20$^h$ 03$^m$ 00.77$^s$ | +28° 18′ 24.7″ | 7.31 | 3.34 | 203 | G5IV | has a planet (b) |
| Z Vul | | | Z | 181987 | 95163 | 19$^h$ 21$^m$ 39.11$^s$ | +25° 34′ 29.4″ | 7.33 | | 626 | B2V+B9V | classical Cepheid, V$_{max}$ = 7.25$^m$, V$_{min}$ = 8.9$^m$, P = 2.454934 d |
| ER Vul | | | ER | 200391 | 103833 | 21$^h$ 02$^m$ 25.91$^s$ | +27° 48′ 26.4″ | 7.37 | | 169.5 | G0V+G5V | W UMa variable, V$_{max}$ = 7.27$^m$, V$_{min}$ = 7.49$^m$, P = 0.69809409 d |
| HD 189733 | | | V452 | 189733 | 98505 | 20$^h$ 00$^m$ 43.71$^s$ | +22° 42′ 39.1″ | 7.67 | 6.26 | 62.9 | K1-K2 | planetary transit and BY Dra variable, ΔV = 0.03$^m$, P = 2.218573 d, has a transiting planet (b) |
| HD 188037 | | | NS | 188037 | | 19$^h$ 52$^m$ 30.08$^s$ | +22° 27′ 14.4″ | 7.76 | | | A2 | slow irregular variable, V$_{max}$ = 7.75$^m$, V$_{min}$ = 8.12$^m$ |
| V Vul | | | V | 340667 | | 20$^h$ 36$^m$ 32.02$^s$ | +26° 36′ 14.5″ | 8.05 | | | G8:Iabv | RV Tau variable, V$_{max}$ = 8.05$^m$, V$_{min}$ = 9.75$^m$, P = 76.07 d |
| HD 201626 | | | | 201626 | 104486 | 21$^h$ 09$^m$ 59.27$^s$ | +26° 36′ 54.9″ | 8.16 | | 738 | C-H2IV: C2 3.5 CH5 CN2.5 | CH star |
| HD 188015 | | | | 188015 | 97769 | 19$^h$ 52$^m$ 04.54$^s$ | +28° 06′ 01.4″ | 8.22 | 4.61 | 172 | G5IV | has a planet (b) |
| HD 203030 | | | V457 | 203030 | 105232 | 21$^h$ 18$^m$ 58.22$^s$ | +26° 13′ 50.0″ | 8.45 | | 133.3 | G8V | BY Dra variable, ΔV = 0.04$^m$, P = 6.664 d, has a planet (b) |
| S Vul | | | S | 338867 | | 19$^h$ 48$^m$ 23.81$^s$ | +27° 17′ 11.4″ | 8.69 | | | K0 | classical Cepheid, V$_{max}$ = 8.69$^m$, V$_{min}$ = 9.42$^m$, P = 68.464 d |
| DR Vul | | | DR | 339770 | | 20$^h$ 13$^m$ 46.85$^s$ | +26° 45′ 01.6″ | 8.71 | | | B8 | Algol variable, V$_{max}$ = 8.65$^m$, V$_{min}$ = 9.27$^m$, P = 2.2508645 d |
| X Vul | | | X | 339279 | 98212 | 19$^h$ 57$^m$ 28.61$^s$ | +26° 33′ 23.3″ | 8.87 | | 23000 | K5 | classical Cepheid, V$_{max}$ = 8.33$^m$, V$_{min}$ = 9.22$^m$, P = 6.319588 d |
| BD+23 3912 | | | | 345957 | 99423 | 20$^h$ 10$^m$ 48.16$^s$ | +23° 57′ 54.5″ | 8.93 | | 315.9 | G0V: | halo star |
| BE Vul | | | BE | 340201 | | 20$^h$ 25$^m$ 33.64$^s$ | +27° 22′ 09.1″ | 9.79 | | | A0 | Algol variable, V$_{max}$ = 9.78$^m$, V$_{min}$ = 11.31$^m$, P = 1.552044 d |
| BP Vul | | | BP | 352179 | 100745 | 20$^h$ 25$^m$ 33.25$^s$ | +21° 02′ 18.0″ | 9.95 | | 2000 | A7 | Algol variable |
| BS Vul | | | BS | 344650 | | 19$^h$ 37$^m$ 26.51$^s$ | +21° 55′ 50.4″ | 10.08 | | | F2 | β Lyr variable, V$_{max}$ = 10.9$^m$, V$_{min}$ = 11.6$^m$, P = 0.47597147 d |
| BO Vul | | | BO | 345287 | | 19$^h$ 56$^m$ 29.07$^s$ | +23° 54′ 45.0″ | 10.12 | | | F0 | Algol variable |
| HAT-P-49 | | | | 340099 | | 20$^h$ 21$^m$ 46.0$^s$ | +26° 41′ 34″ | 10.21 | | 1050 | A5 | has a planet (b) |
| HD 186943 | | | QY | 186943 | 97281 | 19$^h$ 46$^m$ 15.94$^s$ | +28° 16′ 19.1″ | 10.23 | | | WN3+O9.5V | Wolf–Rayet star and eclipsing binary |
| WW Vul | | | WW | 344361 | | 19$^h$ 25$^m$ 58.75$^s$ | +21° 12′ 31.3″ | 10.25 | | | A3 | UX Ori variable, V$_{max}$ = 10.25$^m$, V$_{min}$ = 12.94$^m$ |
| AW Vul | | | AW | 340420 | | 20$^h$ 29$^m$ 01.67$^s$ | +24° 48′ 27.9″ | 11.40 | | | F0 | Algol variable, V$_{max}$ = 10.8$^m$, V$_{min}$ = 11.9$^m$, P = 0.80645141 d |
| Wolf 1346 | | | | 340611 | 101516 | 20$^h$ 34$^m$ 21.88$^s$ | +25° 03′ 49.7″ | 11.55 | | 50.68 | DA2.4 | white dwarf |
| PX Vul | | | PX | | | 19$^h$ 26$^m$ 40.26$^s$ | +23° 53′ 50.9″ | 11.83 | | | F3 | Orion variable, V$_{max}$ = 11.4$^m$, V$_{min}$ = 12.8$^m$ |
| G 185-32 | | | PY | | | 19$^h$ 37$^m$ 13.17$^s$ | +27° 43′ 18.1″ | 12.97 | | | DA | pulsating white dwarf, ΔV = 0.02$^m$ |
| GD 385 | | | PT | | | 19$^h$ 52$^m$ 27.88$^s$ | +25° 09′ 29.1″ | 15.11 | | 124 | DA4.2 | pulsating white dwarf, ΔV = 0.05$^m$ |
| XTE J1859+226 | | | V406 | | | 18$^h$ 58$^m$ 41.58$^s$ | +22° 39′ 29.6″ | | | | G5V-K0V | low-mass X-ray binary |
| TOI-5205 | | | | | | 20$^h$ 55$^m$ 04.91$^s$ | +24° 21′ 38.7″ | 15.9 | | 285 | M4V | has a transiting exoplanet (b) |
| LV Vul | | | LV | | | 19$^h$ 48$^m$ 00.52$^s$ | +27° 10′ 19.3″ | 16.9 | | | | nova, V$_{max}$ = 4.5$^m$, V$_{min}$ = 16.9$^m$ |
| PW Vul | | | PW | | | 19$^h$ 26$^m$ 05.06$^s$ | +27° 21′ 58.8″ | 16.9 | | | | nova, V$_{max}$ = 6.4$^m$, V$_{min}$ = 16.9$^m$ |
| VW Vul | | | VW | | | 20$^h$ 57$^m$ 45.07$^s$ | +25° 30′ 25.7″ | 17.0 | | | | Z Cam variable, V$_{max}$ = 13.1$^m$, V$_{min}$ = 17.0$^m$, P = 0.1687 d |
| QU Vul | | | QU | | | 20$^h$ 26$^m$ 45.94$^s$ | +27° 50′ 42.2″ | 17.9 | | | | nova, V$_{max}$ = 5.3$^m$, V$_{min}$ = 17.9$^m$ |
| NQ Vul | | | NQ | | | 19$^h$ 29$^m$ 14.69$^s$ | +20° 27′ 59.6″ | 18 | | | | nova, V$_{max}$ = 6.01$^m$, V$_{min}$ = 18$^m$ |
| GS 2000+25 | | | QZ | | | 20$^h$ 02$^m$ 49.58$^s$ | +25° 14′ 11.3″ | 18.2 | | | K3V-K6V | X-ray nova |
| V458 Vul | | | V458 | | | 19$^h$ 54$^m$ 24.61$^s$ | +20° 52′ 52.6″ | 18.3 | | | | nova, V$_{max}$ = 8.1$^m$, V$_{min}$ = 18.3$^m$, P = 0.06812255 d |
| QV Vul | | | QV | | | 19$^h$ 04$^m$ 40.32$^s$ | +21° 46′ 14.2″ | 19 | | | | nova, V$_{max}$ = 7$^m$, V$_{min}$ = 19$^m$ |
| CK Vul | | 11 | CK | | | 19$^h$ 47$^m$ 38.1$^s$ | +27° 18′ 48″ | 20.0 | | | | Anthelm's Star; nova, V$_{max}$ = 2.7$^m$, V$_{min}$ = 20.0$^m$ |
| PU Vul | | | PU | | | 20$^h$ 21$^m$ 13.32$^s$ | +21° 34′ 18.7″ | | | | A4II-F8Iab + M6IIIe | nova |
| WR 125 | | | V378 | | | 19$^h$ 28$^m$ 15.62$^s$ | +19° 33′ 21.4″ | | | | WCe+... | Wolf–Rayet star |
| QQ Vul | | | QQ | | | 20$^h$ 05$^m$ 41.91$^s$ | +22° 39′ 58.7″ | | | | M2 | AM Her variable |
| PSR B1919+21 | | | | | | 19$^h$ 21$^m$ 44.81$^s$ | +21° 53′ 02.3″ | | | 2283 | | first pulsar discovered |
| PSR B1930+22 | | | | | | 19$^h$ 32$^m$ 22.86$^s$ | +22° 20′ 52.1″ | | | | | pulsar |
| PSR B1937+21 | | | | | | 19$^h$ 39$^m$ 38.56$^s$ | +21° 35′ 59.1″ | | | | | millisecond pulsar |
| PSR B1953+29 | | | | | | 19$^h$ 55$^m$ 27.88$^s$ | +29° 08′ 43.5″ | | | | | millisecond pulsar |
| PSR B2020+28 | | | | | | 20$^h$ 22$^m$ 37.07$^s$ | +28° 54′ 23.1″ | | | | | pulsar |
| PSR J2007+2722 | | | | | | 20$^h$ 07$^m$ 15.77$^s$ | +27° 22′ 47.7″ | | | 17200 | | pulsar |
| V407 Vul | | | V407 | | | 19$^h$ 14$^m$ 26.09$^s$ | +24° 56′ 44.6″ | | | | | AM CVn variable |
| Table legend:  • Name = Proper name  • B = Bayer designation  • F or/and G. = Flamsteed designation or Gould designation  • Var = Variable star designation  • HD = Henry Draper Catalogue designation number  • HIP = Hipparcos Catalogue designation number  • RA = Right ascension for the Epoch/Equinox J2000.0  • Dec = Declination for the Epoch/Equinox J2000.0  • vis. mag. = visual magnitude (m or m$_v$), also known as apparent magnitude  • abs. mag. = absolute magnitude (M$_v$)  • Dist. (ly) = Distance in light-years from Earth  • Sp. class = Spectral class of the star in the stellar classification system  • Notes = Common name(s) or alternate name(s); comments; notable properties [for example: multiple star status, range of variability if it is a variable star, exoplanets, etc.] |||||||||||||