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 | 6 | 183439 | 95771 | 4.40 | −0.36 | 291 | M1III | Anser;[1] suspected variable, | |||||
23 | 192806 | 99874 | 4.52 | −0.58 | 327 | K3- III Fe-1 | |||||||
(r)[2] | 31 | 198809 | 103004 | 4.56 | 0.77 | 228 | G7IIIa Fe-1 Ba | ||||||
13 | 188260 | 97886 | 4.57 | −0.64 | 359 | B9.5III | |||||||
15 | NT | 189849 | 98543 | 4.66 | 0.49 | 222 | A4III | α² CVn variable, | |||||
1 | 180554 | 94703 | 4.76 | −2.47 | 911 | B4IV | suspected variable, | ||||||
QR | 192685 | 99824 | 4.79 | −3.04 | 1199 | B3V | γ Cas variable, | ||||||
29 | 196724 | 101867 | 4.81 | 0.73 | 213 | A0V | |||||||
12 | V395 | 187811 | 97679 | 4.90 | −1.49 | 619 | B2.5V | Be star, | |||||
30 | 197752 | 102388 | 4.92 | −0.32 | 365 | K2III | |||||||
9 | 184606 | 96275 | 5.00 | −1.35 | 608 | B8IIIn | suspected variable, | ||||||
(q) | 32 | 199169 | 103200 | 5.03 | −1.75 | 739 | K4III | suspected variable, | |||||
28 | 196740 | 101868 | 5.06 | −0.84 | 493 | B5IV | |||||||
17 | 190993 | 99080 | 5.08 | −0.80 | 488 | B3V | |||||||
4 | 182762 | 95498 | 5.14 | 0.84 | 237 | K0III | |||||||
22 | QS | 192713 | 99853 | 5.15 | −5.44 | 4347 | G2Ib SB | Algol variable, | |||||
3 | V377 | 182255 | 95260 | 5.18 | −0.24 | 402 | B6III | 53 Persei variable, | |||||
21 | NU | 192518 | 99738 | 5.19 | 0.18 | 327 | A7IVn | δ Sct variable | |||||
16 | 190004 | 98636 | 5.23 | 1.17 | 211 | F2III | |||||||
24 | 192944 | 99951 | 5.30 | −0.50 | 472 | G8III | |||||||
33 | 199697 | 103511 | 5.30 | −0.13 | 397 | K4III | |||||||
35 | 204414 | 105966 | 5.39 | 1.66 | 182 | A1V | |||||||
2 | ES | 180968 | 94827 | 5.42 | −3.39 | 1918 | B0.5IV | β Cep variable, | |||||
10 | 186486 | 97077 | 5.50 | 0.31 | 356 | G8III | |||||||
25 | 193911 | 100435 | 5.50 | −3.21 | 1801 | B8IIIn | suspected variable, | ||||||
19 | 192004 | 99518 | 5.51 | −2.96 | 1614 | K3II-III | |||||||
18 | 191747 | 99404 | 5.53 | −0.04 | 420 | A3III | δ Sct variable, | ||||||
187982 | 97765 | 5.54 | −3.15 | 1781 | A1Iab | suspected variable, | |||||||
188485 | 97961 | 5.56 | −0.25 | 472 | A0III | variable star, | |||||||
27 | 196504 | 101716 | 5.59 | 0.73 | 305 | B9V | |||||||
5 | 182919 | 95560 | 5.60 | 1.47 | 218 | A0V | |||||||
T | 198726 | 102949 | 5.66 | −2.89 | 1672 | F5Ib | classical Cepheid, | ||||||
194577 | 100754 | 5.66 | −0.43 | 543 | G6III | suspected variable, | |||||||
203925 | 105703 | 5.67 | 1.53 | 220 | A8III | ||||||||
14 | 189410 | 98375 | 5.68 | 2.26 | 158 | F0 | |||||||
203803 | 105652 | 5.70 | 1.98 | 181 | F1IV | ||||||||
178187 | 93845 | 5.78 | 0.74 | 332 | A4III | ||||||||
8 | 183491 | 95785 | 5.82 | −0.04 | 484 | K0III | suspected variable | ||||||
182955 | 95582 | 5.85 | 0.12 | 455 | M0III | slow irregular variable, | |||||||
189944 | 98609 | 5.88 | −0.69 | 672 | B4V | ||||||||
184010 | 96016 | 5.89 | 2.03 | 193 | K0III-IV | suspected variable | |||||||
20 | 192044 | 99531 | 5.91 | −1.81 | 1140 | B7Ve... | variable star, | ||||||
196753 | 101870 | 5.91 | −3.00 | 1976 | K0II-III+.. | ||||||||
187193 | 97402 | 6.00 | 0.56 | 400 | K0II-III | ||||||||
179648 | 94382 | 6.02 | −1.43 | 1006 | A2Vn | ||||||||
196821 | 101919 | 6.08 | −1.19 | 926 | A0III | suspected variable | |||||||
201051 | 104172 | 6.13 | 0.99 | 348 | K0II-III | ||||||||
(3) | 182807 | 95492 | 6.19 | 3.97 | 90 | F7V | |||||||
203858 | 105660 | 6.20 | −0.17 | 612 | A2V | ||||||||
178476 | 93975 | 6.22 | 3.01 | 143 | F3V | ||||||||
191877 | 99479 | 6.24 | −8.55 | 6200 | B1Ib | ||||||||
193094 | 100018 | 6.24 | 0.98 | 367 | G9III | ||||||||
PS | 186518 | 97091 | 6.28 | −4.35 | 4347 | B7V + G1:III | Algol variable, | ||||||
V387 | 176541 | 93270 | 6.28 | −0.55 | 756 | M4III | semiregular variable | ||||||
203206 | 105344 | 6.29 | 0.20 | 539 | B6IV | suspected variable | |||||||
V379 | 187640 | 97572 | 6.29 | −2.13 | 1698 | B5V | rotating ellipsoidal variable, | ||||||
182761 | 95487 | 6.31 | 0.87 | 400 | A0V | ||||||||
184961 | 96417 | 6.33 | 0.11 | 571 | B9sp... | suspected variable | |||||||
7 | 183537 | 95818 | 6.34 | −0.50 | 760 | B5Vn | variable star, | ||||||
203886 | 105689 | 6.35 | 0.39 | 508 | K0III | ||||||||
195692 | 101300 | 6.37 | 1.82 | 264 | Am | ||||||||
182422 | 95340 | 6.40 | −1.30 | 1132 | B9.5V | ||||||||
26 | 196362 | 101641 | 6.40 | −0.26 | 701 | A5III | |||||||
186021 | 96856 | 6.43 | −1.80 | 1442 | K0Iab: | ||||||||
176971 | 93443 | 6.44 | 0.92 | 414 | A4V | ||||||||
190322 | 98772 | 6.45 | 0.46 | 513 | K2 | ||||||||
187614 | 97573 | 6.46 | 0.64 | 475 | G8III | ||||||||
189671 | 98458 | 6.49 | −1.79 | 1475 | G8II | ||||||||
196035 | 101505 | 6.49 | −1.79 | 1475 | B3IV | ||||||||
185436 | 96601 | 6.50 | 0.28 | 572 | K0III | ||||||||
190066 | 98661 | 6.50 | −3.75 | 3663 | B1Iab | ||||||||
BW | 199140 | 103191 | 6.54 | −2.13 | 1772 | B2IIIvar | β Cep variable, | ||||||
LT | 177392 | 93603 | 6.62 | 373 | F2III | δ Sct variable, | |||||||
MW | 192913 | 99927 | 6.64 | 1610 | A0p | α2 CVn variable, | |||||||
SV | 187921 | 97717 | 6.74 | 4100 | G2.5:Iab | classical Cepheid, | |||||||
RS | 180939 | 94822 | 6.85 | 939 | B5V+G0III-IV | Algol variable, | |||||||
195034 | 100963 | 7.09 | 92.04 | G5 | solar twin | ||||||||
U | 185059 | 96458 | 7.15 | 4900 | F5:Iabv | classical Cepheid, | |||||||
190228 | 98714 | 7.31 | 3.34 | 203 | G5IV | has a planet (b) | |||||||
Z | 181987 | 95163 | 7.33 | 626 | B2V+B9V | classical Cepheid, | |||||||
ER | 200391 | 103833 | 7.37 | 169.5 | G0V+G5V | W UMa variable, | |||||||
V452 | 189733 | 98505 | 7.67 | 6.26 | 62.9 | K1-K2 | planetary transit and BY Dra variable,, has a transiting planet (b) | ||||||
NS | 188037 | 7.76 | A2 | slow irregular variable, | |||||||||
V | 340667 | 8.05 | G8:Iabv | RV Tau variable, | |||||||||
201626 | 104486 | 8.16 | 738 | C-H2IV: C2 3.5 CH5 CN2.5 | CH star | ||||||||
188015 | 97769 | 8.22 | 4.61 | 172 | G5IV | has a planet (b) | |||||||
V457 | 203030 | 105232 | 8.45 | 133.3 | G8V | BY Dra variable,, has a planet (b) | |||||||
S | 338867 | 8.69 | K0 | classical Cepheid, | |||||||||
DR | 339770 | 8.71 | B8 | Algol variable, | |||||||||
X | 339279 | 98212 | 8.87 | 23000 | K5 | classical Cepheid, | |||||||
345957 | 99423 | 8.93 | 315.9 | G0V: | halo star | ||||||||
BE | 340201 | 9.79 | A0 | Algol variable, | |||||||||
BP | 352179 | 100745 | 9.95 | 2000 | A7 | Algol variable | |||||||
BS | 344650 | 10.08 | F2 | β Lyr variable, | |||||||||
BO | 345287 | 10.12 | F0 | Algol variable | |||||||||
340099 | 10.21 | 1050 | A5 | has a planet (b) | |||||||||
QY | 186943 | 97281 | 10.23 | WN3+O9.5V | Wolf–Rayet star and eclipsing binary | ||||||||
WW | 344361 | 10.25 | A3 | UX Ori variable, | |||||||||
AW | 340420 | 11.40 | F0 | Algol variable, | |||||||||
340611 | 101516 | 11.55 | 50.68 | DA2.4 | white dwarf | ||||||||
PX | 11.83 | F3 | Orion variable, | ||||||||||
PY | 12.97 | DA | pulsating white dwarf, | ||||||||||
PT | 15.11 | 124 | DA4.2 | pulsating white dwarf, | |||||||||
XTE J1859+226[3] | V406 | G5V-K0V | low-mass X-ray binary | ||||||||||
15.9 | 285 | M4V | has a transiting exoplanet (b) | ||||||||||
LV | 16.9 | nova, | |||||||||||
PW | 16.9 | nova, | |||||||||||
VW | 17.0 | Z Cam variable, | |||||||||||
QU | 17.9 | nova, | |||||||||||
NQ | 18 | nova, | |||||||||||
QZ | 18.2 | K3V-K6V | X-ray nova | ||||||||||
V458 | 18.3 | nova, | |||||||||||
QV | 19 | nova, | |||||||||||
11[4] | CK | 20.0 | Anthelm's Star; nova, | ||||||||||
PU | A4II-F8Iab + M6IIIe | nova | |||||||||||
V378 | WCe+... | Wolf–Rayet star | |||||||||||
M2 | AM Her variable | ||||||||||||
2283 | first pulsar discovered | ||||||||||||
pulsar | |||||||||||||
millisecond pulsar | |||||||||||||
millisecond pulsar | |||||||||||||
pulsar | |||||||||||||
17200 | pulsar | ||||||||||||
V407 | AM CVn variable |