Misplaced Pages

List of stars in Andromeda

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
(Redirected from HD 8375)

This is the list of notable stars in the constellation Andromeda, sorted by decreasing brightness.

Name B F Var HD HIP RA Dec vis.
mag.
abs.
mag.
Dist. (ly) Sp. class Notes
Alpheratz α, (δ) 21 358 677 00 08 23.17 +29° 05′ 27.0″ 2.07 −0.30 97 B9p Alpheratz, Sirrah; α CVn variable, ΔV = 0.04, P = 0.966222 d; spectroscopic binary, also δ Peg
Mirach β 43 6860 5447 01 09 43.80 +35° 37′ 15.0″ 2.07 −1.86 199 M0IIIvar Mirach; variable, has a planet or brown dwarf (b)
γ And γ 57 12533 9640 02 03 53.92 +42° 19′ 47.5″ 2.10 −3.08 355 K3IIb Almach; quadruple star system
δ And δ 31 3627 3092 00 39 19.60 +30° 51′ 40.4″ 3.27 0.81 101 K3III... spectroscopic binary; suspected variable
Andromeda Galaxy (n) 33 00 42 44.31 +41° 16′ 09.4″ 3.44
(nebulous)
2540000 BD+40°148; naked eye spiral galaxy in the Local group
51 And (υ) 51 9927 7607 01 37 59.50 +48° 37′ 42.6″ 3.59 −0.04 174 K3III Nembus; multiple star
ο And ο 1 217675 113726 23 01 55.25 +42° 19′ 33.5″ 3.62 −3.01 692 B6pv SB quadruple star system; γ Cas variable, Vmax = 3.55, Vmin = 3.78
λ And λ 16 222107 116584 23 37 33.71 +46° 27′ 33.0″ 3.81 1.75 84 G8III-IV RS CVn variable, Vmax = 3.65, Vmin = 4.05, P = 53.95 d
μ And μ 37 5448 4436 00 56 45.10 +38° 29′ 57.3″ 3.86 0.75 136 A5V multiple star
ζ And ζ 34 4502 3693 00 47 20.39 +24° 16′ 02.6″ 4.08 0.35 181 K1II β Lyr/RS CVn variable, Vmax = 3.92, Vmin = 4.14, P = 17.7696 d
υ And 50 9826 7513 01 36 47.98 +41° 24′ 23.0″ 4.10 3.45 44 F8V Titawin, has four planets (b, c, d & e)
κ And κ 19 222439 116805 23 40 24.44 +44° 20′ 02.3″ 4.15 0.57 170 B9IVn triple star, has a planet (b)
φ And φ 42 6811 5434 01 09 30.12 +47° 14′ 30.6″ 4.26 −2.51 736 B7III emission-line star
ι And ι 17 222173 116631 23 38 08.18 +43° 16′ 05.1″ 4.29 −1.65 502 B8V Keff al Salsalat, Manus Catenata
π And π 29 3369 2912 00 36 52.84 +33° 43′ 09.7″ 4.34 −2.18 656 B5V spectroscopic binary; suspected variable
ε And ε 30 3546 3031 00 38 33.50 +29° 18′ 44.5″ 4.34 0.77 169 G5III...
η And η 38 5516 4463 00 57 12.43 +23° 25′ 03.9″ 4.40 0.04 243 G8III-IV spectroscopic binary
σ And σ 25 1404 1473 00 18 19.71 +36° 47′ 07.2″ 4.51 1.33 141 A2V suspected variable
ν And ν 35 4727 3881 00 49 48.83 +41° 04′ 44.2″ 4.53 −2.06 679 B5V SB spectroscopic binary
7 And 7 219080 114570 23 12 32.92 +49° 24′ 21.5″ 4.53 2.58 80 F0V
θ And θ 24 1280 1366 00 17 05.54 +38° 40′ 54.0″ 4.61 0.16 253 A2V suspected variable
3 And 3 218031 113919 23 04 10.83 +50° 03′ 06.1″ 4.64 0.94 179 K0III
65 And 65 14872 11313 02 25 37.40 +50° 16′ 43.2″ 4.73 −0.39 345 K4III triple star
58 And 58 13041 9977 02 08 29.15 +37° 51′ 33.1″ 4.78 0.86 198 A5IV-V
8 And 8 219734 115022 23 17 44.62 +49° 00′ 55.0″ 4.82 −1.69 655 M2III suspected variable
ω And ω 48 8799 6813 01 27 39.09 +45° 24′ 25.0″ 4.83 2.57 92 F5IV
γ And γ 57 12534 02 03 54.70 +42° 19′ 51.0″ 4.84 -0.3 350 B8V component of the γ And system; triple star system
60 And b 60 13520 10340 02 13 13.34 +44° 13′ 54.1″ 4.84 −1.32 556 K4III suspected variable
ξ And ξ 46 8207 6411 01 22 20.39 +45° 31′ 43.5″ 4.87 0.98 195 K0III-IV Adhil
τ And τ 53 10205 7818 01 40 34.80 +40° 34′ 37.6″ 4.96 −1.64 681 B8III suspected variable
41 H. And υ 10307 7918 01 41 46.52 +42° 36′ 49.7″ 4.96 4.45 41 G2V spectroscopic binary
ψ And ψ 20 223047 117221 23 46 02.04 +46° 25′ 13.0″ 4.97 −3.05 1309 G5Ib multiple star
22 And 22 571 841 00 10 19.24 +46° 04′ 20.2″ 5.01 −2.44 1006 F2II
χ And χ 52 10072 7719 01 39 21.02 +44° 23′ 10.1″ 5.01 0.66 242 G8III...
41 And (d) 41 6658 5317 01 08 00.72 +43° 56′ 32.1″ 5.04 1.14 196 A3m
2 And 2 217782 113788 23 02 36.34 +42° 45′ 28.1″ 5.09 −0.06 349 A3Vn multiple star
V428 And V428 3346 2900 00 36 46.47 +44° 29′ 18.6″ 5.14 −1.38 656 K5III semiregular variable, ΔV = 0.06, P = 11.5 d; has a possible planetary system
ρ And ρ 27 1671 1686 00 21 07.23 +37° 58′ 07.3″ 5.16 1.71 160 F5III
HD 2421 2421 2225 00 28 13.59 +44° 23′ 40.2″ 5.18 0.63 265 A2Vs spectroscopic binary
64 And 64 14770 11220 02 24 24.89 +50° 00′ 23.9″ 5.19 −0.11 375 G8III
GN And 28 GN 2628 2355 00 30 07.34 +29° 45′ 06.1″ 5.20 1.43 185 A7III low-amplitude δ Sct variable, ΔV = 0.05, P = 0.0693041 d
14 And 14 221345 116076 23 31 17.20 +39° 14′ 11.0″ 5.22 0.80 249 K0III Veritate, suspected variable; has a planet (b)
49 And A 49 9057 6999 01 30 06.10 +47° 00′ 26.6″ 5.27 0.53 290 K0III
32 And 32 3817 3231 00 41 07.20 +39° 27′ 31.2″ 5.30 0.18 344 G8III
4 And 4 218452 114200 23 07 39.28 +46° 23′ 14.3″ 5.30 0.20 342 K5III double star
6 Per (6) 13530 10366 02 13 36.02 +51° 03′ 58.4″ 5.31 1.38 199 G8III:var spectroscopic binary; suspected variable
62 And c 62 14212 10819 02 19 16.85 +47° 22′ 48.0″ 5.31 0.84 255 A1V
18 And 18 222304 116709 23 39 08.35 +50° 28′ 18.3″ 5.35 −0.04 390 B9V
55 And 55 11428 8814 01 53 17.35 +40° 43′ 47.3″ 5.42 −0.67 540 K1III double star
11 And 11 219945 115152 23 19 29.79 +48° 37′ 30.7″ 5.44 0.43 328 K0III
3421 2942 00 37 21.23 +35° 23′ 58.2″ 5.45 −2.03 1022 G5III
36 And 36 5286 4288 00 54 58.02 +23° 37′ 42.4″ 5.46 2.51 127 K1IV suspected variable
V340 And 15 V340 221756 116354 23 34 37.55 +40° 14′ 11.6″ 5.55 1.28 233 A1III low-amplitude δ Sct variable, ΔV = 0.007
PZ And 63 PZ 14392 10944 02 20 58.17 +50° 09′ 05.5″ 5.57 0.38 356 B9p Si α CVn variable, ΔV = 0.05, P = 4.189 d
47 And 47 8374 6514 01 23 40.56 +37° 42′ 54.0″ 5.60 1.54 211 A1m
10204 7825 01 40 39.56 +43° 17′ 51.9″ 5.63 1.05 268 A9IV:
44 And 44 6920 5493 01 10 18.85 +42° 04′ 53.7″ 5.67 2.06 172 F8V
5 And 5 218470 114210 23 07 45.25 +49° 17′ 43.6″ 5.68 3.02 111 F5V
HD 5788 5788 4675 01 00 03.55 +44° 42′ 47.9″ 5.69 0.14 420 A2Vn binary star with HD 5789
56 And 56 11749 9021 01 56 09.23 +37° 15′ 06.5″ 5.69 0.73 320 G8III... multiple star
23 And 23 905 1086 00 13 30.94 +41° 02′ 08.6″ 5.71 2.99 114 F0IV
HD 16028 16028 12072 02 35 38.74 +37° 18′ 44.2″ 5.72 −0.86 676 K4III triple star
V388 And 13 V388 220885 115755 23 27 07.33 +42° 54′ 43.1″ 5.75 0.97 294 B9III α CVn variable, Vmax = 5.73, Vmin = 5.77, P = 1.47931 d
12 And 12 220117 115280 23 20 53.17 +38° 10′ 56.9″ 5.77 2.63 138 F5V triple star
1632 1657 00 20 45.54 +32° 54′ 40.4″ 5.79 −0.69 646 K5III
45 And 45 7019 5550 01 11 10.29 +37° 43′ 26.9″ 5.80 −1.44 916 B7III-IV double star
HD 14622 14622 11090 02 22 50.36 +41° 23′ 47.5″ 5.81 2.44 154 F0III-IV has two optical companions
10 And 10 219981 115191 23 19 52.38 +42° 04′ 40.9″ 5.81 −0.30 542 M0III
HD 222109 222109 116582 23 37 32.03 +44° 25′ 44.5″ 5.81 −1.20 823 B8V double star
HD 224635 224635 118281 23 59 29.33 +33° 43′ 26.9″ 5.81 3.50 95 F8 multiple star
OU And OU 223460 117503 23 49 40.96 +36° 25′ 31.4″ 5.86 0.21 440 G1IIIe FK Com variable, ΔV = 0.07, P = 24.2 d
1439 1493 00 18 38.22 +31° 31′ 02.0″ 5.88 −0.23 543 A0IV
HD 2767 2767 2475 00 31 25.61 +33° 34′ 54.1″ 5.88 0.10 467 K1III... binary star
HD 1606 1606 1630 00 20 24.39 +30° 56′ 08.2″ 5.89 −0.37 582 B7V suspected variable
11727 9001 01 55 54.47 +37° 16′ 40.1″ 5.89 −1.52 991 K5III optical component of 56 And
KK And KK 9531 7321 01 34 16.60 +37° 14′ 13.9″ 5.90 0.50 392 B8Vp(Si) α CVn variable, ΔV = 0.012, P = 0.6684 d
16176 12181 02 36 57.08 +38° 44′ 02.3″ 5.91 2.24 177 F5V
6 And 6 218804 114430 23 10 27.36 +43° 32′ 41.1″ 5.91 3.65 112 F5V Astrometric binary
10975 8423 01 48 38.84 +37° 57′ 10.6″ 5.94 1.06 308 K0III
39 And 39 6116 4903 01 02 54.28 +41° 20′ 42.7″ 5.95 0.84 344 A5m double star
8671 6711 01 26 18.60 +43° 27′ 28.4″ 5.98 2.90 135 F7V
AN And 9 AN 219815 115065 23 18 23.33 +41° 46′ 25.3″ 5.98 0.17 472 A7m β Lyr variable, Vmax = 5.96, Vmin = 6.11, P = 3.21952 d
HD 5608 5608 4552 00 58 14.19 +33° 57′ 03.8″ 5.99 2.17 190 K0 has a transiting planet (b)
224165 117956 23 55 33.48 +47° 21′ 21.0″ 6.01 −2.46 1614 G8Ib
224342 118071 23 57 03.63 +42° 39′ 29.7″ 6.01 −2.22 1442 F8III
4335 3604 00 46 10.80 +44° 51′ 41.4″ 6.03 0.32 452 B9.5IIIMNp.
13594 10403 02 14 02.53 +47° 29′ 03.8″ 6.05 2.96 135 F5V
HD 3883 3883 3269 00 41 35.98 +24° 37′ 44.6″ 6.06 0.30 462 A7m suspected variable
V439 And V439 166 544 00 06 36.53 +29° 01′ 19.0″ 6.07 5.39 45 K0V BY Draconis variable, ΔV = 0.04, P = 6.23 d
5118 4185 00 53 28.22 +37° 25′ 05.9″ 6.07 0.77 374 K3III:
221293 116030 23 30 39.54 +38° 39′ 44.0″ 6.07 −0.33 621 G9III
HD 223229 223229 117340 23 47 33.05 +46° 49′ 57.3″ 6.08 −1.96 1320 B3IV suspected variable
225239 394 00 04 53.21 +34° 39′ 34.4″ 6.09 3.26 120 G2V
59 And A 59 13294 10176 02 10 52.83 +39° 02′ 22.5″ 6.09 1.56 263 B9V binary star
26 And 26 1438 1501 00 18 42.15 +43° 47′ 28.1″ 6.10 −0.53 692 B8V double star
5526 4501 00 57 39.64 +45° 50′ 21.8″ 6.10 0.45 439 K2III
HD 225218 225218 365 00 04 36.60 +42° 05′ 33.2″ 6.11 −2.45 1680 B9III double star
7647 5993 01 17 05.05 +44° 54′ 07.5″ 6.11 −0.18 590 K5
HD 1185 1185 1302 00 16 21.50 +43° 35′ 42.4″ 6.12 1.28 303 A2V double star
218416 114162 23 07 10.05 +52° 48′ 59.6″ 6.12 0.55 423 K0III
GO And GO 4778 3919 00 50 18.21 +45° 00′ 08.1″ 6.13 1.34 296 A0p... α CVn variable, ΔV = 0.04, P = 2.5481 d
7158 5650 01 12 34.06 +45° 20′ 14.9″ 6.13 −0.52 698 M1III
66 And 66 15138 11465 02 27 51.75 +50° 34′ 12.7″ 6.16 2.54 173 F4V spectroscopic binary
14372 10924 02 20 41.50 +47° 18′ 39.0″ 6.17 −0.87 836 B5V
743 967 00 11 59.03 +48° 09′ 08.5″ 6.18 0.05 550 K4III
3411 2926 00 37 07.20 +24° 00′ 51.3″ 6.18 1.13 334 K2III
HD 221776 221776 116365 23 34 46.73 +38° 01′ 26.3″ 6.18 −0.41 678 K5 double star
16327 12287 02 38 17.86 +37° 43′ 36.6″ 6.19 1.60 270 F6III triple star
HD 221246 221246 115996 23 30 07.39 +49° 07′ 59.3″ 6.19 −0.91 856 K5III member of the NGC 7686 star cluster
OP And OP 9746 7493 01 36 27.21 +48° 43′ 22.2″ 6.20 0.65 420 K1III: BY Dra variable, ΔV = 0.09
400 699 00 08 41.02 +36° 37′ 38.7″ 6.21 3.61 108 F8IV
14213 10814 02 19 10.84 +46° 28′ 20.2″ 6.21 0.50 452 A4V
952 1123 00 14 02.29 +33° 12′ 21.9″ 6.22 1.45 293 A1V
HD 895 895 1076 00 13 23.93 +26° 59′ 15.4″ 6.24 0.78 403 G0III triple star
222451 116824 23 40 40.47 +36° 43′ 14.6″ 6.24 3.01 144 F1V
224906 137 00 01 43.85 +42° 22′ 01.7″ 6.25 −1.80 1331 B9IIIp Mn
11613 8922 01 54 53.75 +40° 42′ 07.9″ 6.25 1.13 345 K2
HD 220105 220105 115261 23 20 44.11 +44° 06′ 58.5″ 6.25 1.73 261 A5Vn double star
221661 116292 23 33 42.99 +45° 03′ 29.1″ 6.25 0.12 548 G8II
HD 2942 2942 2583 00 32 49.09 +28° 16′ 48.8″ 6.26 0.47 469 G8II triple star
8774 6776 01 27 06.21 +34° 22′ 39.3″ 6.27 3.12 139 F7IVsvar
2507 2270 00 28 56.67 +36° 53′ 58.9″ 6.28 0.51 464 G5III
8375 6512 01 23 37.31 +34° 14′ 44.2″ 6.28 2.43 192 G8IV
11624 8930 01 54 57.63 +37° 07′ 42.0″ 6.28 0.25 525 K0
7758 6087 01 18 10.14 +47° 25′ 11.0″ 6.29 −2.07 1531 K0
16350 12305 02 38 27.94 +38° 05′ 21.0″ 6.29 −0.47 734 B9.5V
219962 115171 23 19 41.37 +48° 22′ 51.1″ 6.29 0.47 475 K1III
217314 113501 22 59 10.37 +52° 39′ 16.0″ 6.31 −0.26 672 K2
10597 8127 01 44 26.53 +46° 08′ 23.2″ 6.32 0.23 540 K5III
219290 114714 23 14 14.34 +50° 37′ 04.5″ 6.32 0.82 411 A0V
10486 8044 01 43 16.39 +45° 19′ 21.5″ 6.33 2.61 181 K2IV
10874 8370 01 47 48.00 +46° 13′ 47.6″ 6.33 2.50 190 F6V
1075 1208 00 15 06.93 +31° 32′ 08.7″ 6.34 −1.70 1320 K5
HD 8673 8673 6702 01 26 08.62 +34° 34′ 47.7″ 6.34 3.43 125 F7V has a planet (b)
1083 1215 00 15 10.55 +27° 17′ 00.5″ 6.35 0.84 412 A1Vn double star
1527 1575 00 19 41.58 +40° 43′ 46.2″ 6.35 0.25 541 K1III
221970 116505 23 36 30.52 +32° 54′ 15.1″ 6.35 1.92 251 F6V
CG And CG 224801 63 00 00 43.62 +45° 15′ 12.0″ 6.36 −0.23 678 B9p SiEu α CVn variable, Vmax = 6.32, Vmin = 6.42, P = 3.73975 d
HD 16004 16004 12057 02 35 27.89 +39° 39′ 52.1″ 6.36 0.11 580 B9MNp... triple star
13818 10562 02 15 57.69 +47° 48′ 43.4″ 6.37 0.61 462 G9III-IV
LN And LN 217811 113802 23 02 45.15 +44° 03′ 31.6″ 6.37 −1.42 1177 B2V double star; not variable despite designation
V385 And V385 220524 115530 23 24 08.88 +41° 36′ 46.3″ 6.37 −1.55 1249 M0 irregular variable, Vmax = 6.36, Vmin = 6.47
GY And GY 9996 7651 01 38 31.84 +45° 23′ 58.9″ 6.38 0.66 455 B9Vp (Cr-Eu) Promethium lines; α CVn variable, Vmax = 6.27, Vmin = 6.44, P = 8000 d
13013 9983 02 08 33.55 +44° 27′ 34.4″ 6.38 0.78 430 G8III
218365 114152 23 07 04.99 +35° 38′ 11.3″ 6.38 −0.08 638 K0
9712 7444 01 35 52.46 +41° 04′ 35.1″ 6.39 1.01 388 K1III
V529 And V529 8801 6794 01 27 26.67 +41° 06′ 04.0″ 6.42 2.69 182 Am... δ Scuti variable, ΔV = 0.03, P = 0.40331 d
217731 113750 23 02 11.32 +44° 34′ 22.4″ 6.43 1.22 359 K0
HD 222641 222641 116941 23 42 14.68 +44° 59′ 30.3″ 6.43 −0.48 786 K5III suspected variable
HD 7853 7853 6140 01 18 47.02 +37° 23′ 10.7″ 6.44 0.71 456 A5m double star
14221 10830 02 19 22.77 +48° 57′ 19.0″ 6.44 2.39 210 F4V
219668 114981 23 17 16.59 +45° 09′ 51.5″ 6.44 2.10 241 K0IV
HD 6114 6114 4911 01 03 01.47 +47° 22′ 34.3″ 6.46 1.39 337 A9V double star
11884 9163 01 57 59.23 +47° 05′ 43.9″ 6.48 −1.24 1140 K0
ET And ET 219749 115036 23 17 55.99 +45° 29′ 20.2″ 6.48 0.36 545 B9Vp(Si) α CVn variable, ΔV = 0.03, P = 1.61888 d
HD 222399 222399 116781 23 40 02.82 +37° 39′ 10.2″ 6.49 1.74 291 F2IV double star
PY And PY 3322 2865 00 36 20.00 +27° 15′ 17″ 6.50 -0.16 701 B8IIImnp... α CVn variable, ΔV = ~0.03
800 1009 00 12 34.08 +44° 42′ 26.1″ 6.50 0.50 517 K0
59 And B 59 13295 10180 02 10 53.67 +39° 02′ 36.0″ 6.82 −1.76 1698 A1Vn component of the 59 And system
HD 222155 222155 116616 23 38 00 +48° 59′ 47″ 7.1 3.65 160 G2V has a planet (b)
HD 16175 16175 12191 02 37 01.91 +42° 03′ 45.5″ 7.28 3.40 195 G0 Buna; has a planet (b)
R And R 1967 1901 00 24 01.95 +38° 34′ 37.3″ 7.39 -5.19 790 S6.5IIIeZr6Ti2 Mira variable, Vmax = 5.8, Vmin = 15.2, P = 409.2 d
HD 1605 1605 1640 00 20 32.0 +30° 58′ 29″ 7.52 2.88 276 K1IV has two planets (b & c)
HD 13931 13931 10626 02 16 47.38 +43° 46′ 22.8″ 7.52 4.3 144 G0 has a planet (b)
HD 5583 5583 00 57 57.0 +34° 59′ 08″ 7.6 0.88 721 K0 has a planet (b)
RW And RW 4489 00 47 18.92 +32° 41′ 08.6″ 7.9 -0.52 1375 M5e-M10e(S6,2e) Mira variable, Vmax = 7.9, Vmin = 15.7, P = 430 d
Groombridge 34 1326 1475 00 18 22.9 +44° 01′ 22″ 8.01 10.25 11.62 M6Ve + M1Ve 16th closest star system, binary; both components GQ and GX And flare stars
HD 15082 15082 11397 02 26 51.06 +37° 33′ 01.7″ 8.3 3.0 377 A5 has a transiting planet WASP-33b
RU And RU 01 38 37 38° 40′ 12″ 9.9 M5e-M6e a variable star in the constellation of Andromeda. It is classified as a semiregular variable pulsating giant star, and varies from an apparent visual magnitude of 14.5 at minimum brightness to a magnitude of 9.9 at maximum brightness, with a period of approximately 238.3 days.
Y And 10112 01 39 36.89 +39° 20′ 35″ 10.39 8,000 M3-4.5e Mira Cet variable
Z And Z 221650 116287 23 33 39.95 +48° 49′ 05.9″ 10.53 2.38 1393 M2III + B1eq prototype of Z And variables, Vmax = 7.7, Vmin = 11.3
HAT-P-6 23 39 05.81 +42° 27′ 57.5″ 10.54 4.03 650 F Sterrennacht; has a transiting planet (b)
HAT-P-16 00 38 17.56 +42° 27′ 47.2″ 10.8 3.9 766 F8 has a transiting planet (b)
HAT-P-32 02 01 10 +46° 41′ 16″ 11.29 3.76 1044 F/G has a transiting planet (b)
WASP-1 00 20 40.08 +31° 59′ 23.8″ 11.79 3.89 1239 F7V has a transiting planet (b)
Ross 248 23 41 54.99 +44° 10′ 40.8″ 12.29 14.79 10.32 M6e HH And; 8th closest star system, flare star
HAT-P-19 00 38 04 +34° 42′ 42″ 12.9 6.24 701 K has a transiting planet (b)
HAT-P-28 00 52 00 +34° 43′ 42″ 13.03 5.05 1288 G3 has a transiting planet (b)
HAT-P-53 01 27 29.0 +38° 58′ 05″ 13.73 4.45 2345 has a transiting planet (b)
S And S 00 42 43.11 +41° 16′ 04.2″ 2600000 Ia SN 1885A; BD+40°147a; type Ia supernova in the Andromeda Galaxy, Vmax = 5.8, Vmin = < 16
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 mv), also known as apparent magnitude
 • abs. mag. = absolute magnitude (Mv)
 • 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

Notes
  1. It was commonly with δ Peg by Bayer.
  2. Flamsteed lettered it as n.
  3. Armando Gil de Paz et al., "The GALEX Ultraviolet Atlas of Nearby Galaxies," The Astrophysical Journal Supplement Series (ApJS), American Astronomical Society, 2007, 173 185–255.
  4. Bayer designated it as υ Per.
  5. Bode lettered it as 2.υ, in his "Verzeichniss".
  6. Flamsteed lettered it as υ.
  7. Bode lettered it as 1.υ in his "Verzeichniss".
  8. ^ Final Results of NameExoWorlds Public Vote Released
  9. E.B Knobel – On a catalogue of stars in the Calendarium of Al Achsasi Al Mouakket
  10. ^ Flamsteed unlettered it in his catalogue and atlas.
  11. Bayer originally lettered it as υ.
  12. Flamsteed lettered it as λ.
  13. Flamsteed lettered it as d.
  14. Flamsteed lettered it as ξ.
  15. Flamsteed lettered it as h Per.
  16. Persei, on the constellation boundary between Andromeda with Perseus
  17. RU And, database entry, Combined General Catalog of Variable Stars (GCVS4.2, 2004 Ed.), N. N. Samus, O. V. Durlevich, et al., CDS ID II/250 Accessed on line 2009-06-30.
  18. V* RU And -- Semiregular Pulsating Variable Star, database entry, SIMBAD. Accessed on line 2009-06-30.

See also

References

Lists of stars by constellation
  • List of stars in ...
Constellation of Andromeda
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star
clusters
NGC
Other
Nebulae
NGC
Galaxies
Messier
NGC
Numbered
Other
Galaxy clusters
Astronomical events
Category
Categories: