Stand 2017 sind über 52.011 veränderliche Sterne bekannt [ 1 ] , und es werden regelmäßig neue entdeckt. Daher ist eine vollständige Liste aller veränderlichen Sterne an dieser Stelle nicht möglich (vgl. GCVS ). Im Folgenden finden Sie eine Liste bekannter, heller, bedeutender oder anderweitig interessanter veränderlicher Sterne .
| Bezeichnung (Name) | Konstellation | Entdeckung | Scheinbare Helligkeit (Maximum) [ 2 ] | Scheinbare Helligkeit (Minimum) [ 3 ] | Größenbereich | Zeitraum | Typ | Kommentar |
|---|---|---|---|---|---|---|---|---|
| R und | Andromeda | 5 m .8 | 14 m .9 | 9.1 | 409 d | Mira-Variable (M) | ||
| S And ( Supernova 1885) | Ernst Hartwig , 20. August 1885 | 5 m .8 | 16 m | 10.2 | Supernova (SNI) | |||
| U Ant | Antlia | 8 m .1 (p) | 9 m .7 (p) | 1.6 | LB | |||
| θ Aps | Apus | 6 m .4 (p) | 8 m .6 (p) | 2.2 | 119 d | Halbregulär (SRB) | ||
| η Aql | Adler | Pigott , 1784 | 3 m .48 | 4 m .39 | 0,91 | 7,17664 d | Klassischer Cepheiden (DCEP) | |
| R Aql | 5 m .5 | 12 m .0 | 6,5 | 284 d | Mira-Variable (M) | |||
| V Aql | 6 m .6 | 8 m .4 | 1.8 | 353 d | Halbregulär (SRB) | |||
| R Aqr | Wassermann | Karl Ludwig Harding , 1810 | 5 m .8 | 12 m .4 | 6.9 | 387 d | Mira-Variable (M) | |
| T Aqr | 7 m .2 | 14 m .2 | 7.0 | 202 d | Mira-Variable (M) | |||
| U Ara | Ara | 7 m .7 | 14 m .1 | 6.4 | 225 d | Mira-Variable (M) | ||
| R Ari | Widder | 7 m .4 | 13 m .7 | 6.3 | 187 d | Mira-Variable (M) | ||
| U Ari | 7 m .2 | 15 m .2 | 8.0 | 371 d | Mira-Variable (M) | |||
| ε Aur (Almaaz) | Fuhrmann | Johann Heinrich Fritsch, 1821 | 2 m .92 | 3 m .83 | 0,91 | 27,08 Jahre | Bedeckungsveränderlicher vom Algol-Typ (EA/GS) | |
| R Aur | 6 m .7 | 13 m .9 | 7.2 | 458 d | Mira-Variable (M) | |||
| AE Aur | 5 m .78 | 6 m .08 | 0,30 | Orion-Veränderlicher (INA) | ||||
| R Boo | Boötes | 6 m .2 | 13 m .1 | 6.9 | 223 d | Mira-Variable (M) | ||
| W Boo | 4 m .73 | 5 m .4 | 0,67 | 450 d | Halbregulär (SRB:) | |||
| X-Kamera | Camelopardalis | 7 m .4 | 14 m .2 | 6.8 | 144 d | Mira-Variable (M) | ||
| VZ-Kamera | 4 m .80 | 4 m .96 | 0,16 | 23,7 Tage | Halbregulär (SR) | |||
| R-Kappe | Steinbock | Hind , 1848 | 9 m .4 | 14 m .9 | 5,5 | 345 d | Mira-Variable (M) | |
| η Auto | Carina | Burchell , 1827 | -0 m .8 | 7 m .9 | 8.6 | S Doradus (SDOR) | "Der unberechenbare Supergigant" | |
| l Auto | 3 m .28 | 4 m .18 | 0,90 | 35,53584 d | Klassischer Cepheiden (DCEP) | |||
| R Auto | 3 m .9 | 10 m .5 | 6.6 | 309 d | Mira-Variable (M) | |||
| Narbe | 4 m .5 | 9 m .9 | 5.4 | 149 d | Mira-Variable (M) | |||
| γ Cas (Tiansi) | Kassiopeia | 1 m .6 | 3 m .0 | 1.4 | Gamma Cassiopeiae (GCAS) | |||
| R Cas | 4 m .7 | 13 m .5 | 8.9 | 430 d | Mira-Variable (M) | |||
| S Cas | 7 m .9 | 16 m .1 | 8.2 | 612 d | Mira-Variable (M) | |||
| W Cas | 7 m .8 | 12 m .5 | 4.7 | 406 d | Mira-Variable (M) | |||
| WZ Cas | 6 m .3 | 8 m .5 | 2.2 | Halbregulär (SRB) | Visueller Doppelstern, durch ein Fernglas sichtbar | |||
| R Cen | Centaurus | 5 m .3 | 11 m .8 | 6,5 | 546 d | Mira-Variable (M) | ||
| S Cen | 9 m .2 (p) | 10 m .7 (p) | 1,5 | 65 Tage | Halbregulär (SR) | |||
| T Cen | 5 m .5 | 9 m .0 | 3,5 | 90,44 d | Semireguläre (SRA) | |||
| V645 Cen ( Proxima Centauri ) | 12 m .1 (B) | 13 m .12 (B) | 1.02 | UV Ceti (UV) | ||||
| δ Cep | Kepheus | John Goodricke , 1784 | 3 m .48 | 4 m .37 | 0,89 | 5,36634 d | Klassischer Cepheid- Prototyp (DCEP). | Doppelstern, im Fernglas sichtbar |
| Vega | Lyra | -0 m .02 | 0 m .07 | 0,09 | 0,107 d | Delta Scuti Variable | Hellster veränderlicher Stern am Himmel. | |
| μ Cep (Herschels Granatstern) | Kepheus | William Herschel , 1782 | 3 m .43 | 5 m .1 | 1,67 | 730 d | Halbregulär (SRC) | |
| S Cep | Kepheus | 7 m .4 | 12 m .9 | 5,5 | 487 d | Mira-Variable (M) | ||
| T Cep | 5 m .2 | 11 m .3 | 6.1 | 388 d | Mira-Variable (M) | |||
| U Cep | 6 m .75 | 9 m .24 | 2,49 | 2,49305 d | Bedeckungsveränderlicher vom Algol-Typ (EA/SD) | |||
| SS Cep | 8 m .0 (p) | 9 m .1 (p) | 1.1 | 90 Tage | Halbregulär (SRB) | |||
| ST Cep | 7 m .8 | Keiner | Mira-Variable (M) | |||||
| AR Cep | 7 m .0 | 7 m .9 | 0,9 | Halbregulär (SRB) | ||||
| o Cet ( Mira ) | Walfische | David Fabricius , 1596; die Variabilität wurde möglicherweise erstmals von Johannes Fokkes Holwarda , 1638, festgestellt. | 2 m .0 | 10 m .1 | 8.1 | 332 d | Mira-Variable (M) | „Das Wunder“ – der erste entdeckte nicht-ephemere/kataklysmische veränderliche Stern. |
| T Cet | 5 m .0 | 6 m .9 | 1.9 | 159 d | Halbregulär (SRC) | |||
| U Cet | 6 m .8 | 13 m .4 | 6.6 | 235 d | Mira-Variable (M) | |||
| W Cet | 7 m .1 | 14 m .8 | 7,7 | 351 d | Mira-Variable (M) | |||
| R Cha | Chamäleon | 7 m .5 | 14 m .2 | 6.7 | 335 d | Mira-Variable (M) | ||
| R CMa | Canis Major | 5 m .70 | 6 m .34 | 0,64 | 1,13594 d | Bedeckungsveränderlicher vom Algol-Typ (EA/SD) | ||
| VY CMa | 6 m .5 | 9 m .6 | 3.1 | einzigartig (*) | ||||
| FW CMa | 5 m .00 | 5 m .50 | 0,50 | Gamma Cassiopeiae (GCAS) | ||||
| S CMi | 6 m .6 | 13 m .2 | 6.6 | 333 d | Mira-Variable (M) | |||
| R CNC | Krebs | 6 m .07 | 11 m .8 | 5,73 | 362 d | Mira-Variable (M) | ||
| S CNC | Hind , 1848 | 8 m .29 | 10 m .25 | 1,96 | 9,48455 d | Bedeckungsveränderlicher vom Algol-Typ (EA/DS) | ||
| T CNC | Hind , 1850 | 7 m .6 | 10 m .5 | 2.9 | 482 d | Halbregulär (SRB) | ||
| X CNC | 5 m .6 | 7 m .5 | 1.9 | 195 d | Halbregulär (SRB) | |||
| T Col | Columba | 6 m .6 | 12 m .7 | 6.1 | 226 d | Mira-Variable (M) | ||
| R Com | Coma Berenices | 7 m .1 | 14 m .6 | 7,5 | 363 d | Mira-Variable (M) | ||
| α CrB (Alphecca oder Gemma) | Corona Borealis | 2 m .21 (B) | 2 m .32 (B) | 0,11 | 17,35991 d | Bedeckungsveränderlicher vom Algol-Typ (EA/DM) | ||
| R CrB | Piggott , 1795 | 5 m .71 | 14 m .8 | 9.09 | R Coronae Borealis (RCB) | |||
| S CrB | 5 m .8 | 14 m .1 | 8,7 | 360 d | Mira-Variable (M) | |||
| T CrB (Blaze Star) | 2 m .0 | 10 m .8 | 8.8 | (80 Jahre) | recurrent nova (NR) | |||
| U CrB | 7 m .66 | 8 m .79 | 1.13 | 3,45220 d | Bedeckungsveränderlicher vom Algol-Typ (EA/SD) | |||
| V CrB | 6 m .9 | 12 m .6 | 5.3 | 358 d | Mira-Variable (M) | |||
| W CrB | 7 m .8 | 14 m .3 | 6,5 | 238 d | Mira-Variable (M) | |||
| R Cru | Kern | 6 m .40 | 7 m .23 | 0,83 | 5,82575 d | Klassischer Cepheiden (DCEP) | ||
| R Crv | Rabe | 6 m .7 | 14 m .4 | 7,7 | 317 d | Mira-Variable (M) | ||
| χ Cyg | Schwan | Kirch , 1686 | 3 m .3 | 14 m .2 | 10.9 | 408 d | Mira-Variable (M) | |
| R Cyg | 6 m .1 | 14 m .4 | 8.3 | 426 d | Mira-Variable (M) | |||
| U Cyg | 5 m .9 | 12 m .1 | 6.2 | 463 d | Mira-Variable (M) | |||
| W Cyg | 6 m .80 (B) | 8 m .9 (B) | 2.1 | 131 d | Halbregulär (SRB) | |||
| X Cyg | 5 m .85 | 6 m .91 | 1.06 | 16.38633 d | Klassischer Cepheiden (DCEP) | |||
| RT Cyg | 6 m .0 | 13 m .1 | 7.1 | 190 d | Mira-Variable (M) | |||
| SS Cyg | 7 m .7 | 12 m .4 | 4.7 | (49,5 d) | Zwergnova UGSS-Prototyp | |||
| SU Cyg | 6 m .44 | 7 m .22 | 0,78 | 3,84555 d | Klassischer Cepheiden (DCEP) | |||
| CH Cyg | 5 m .60 | 8 m .49 | 2,89 | Z Andromedae (ZAND+SR) | ||||
| R Del | Delphinus | 7 m .6 | 13 m .8 | 6.2 | 285 d | Mira-Variable (M) | ||
| U Del | 7 m .6 (p) | 8 m .9 (p) | 1.3 | 110 d | Halbregulär (SRB) | |||
| EU-Delegation | 5 m .79 | 6 m .9 | 1.11 | 59,7 d | Halbregulär (SRB) | |||
| β Dor | Dorado | 3 m .46 | 4 m .08 | 0,62 | 9,8426 d | Klassischer Cepheiden (DCEP) | ||
| S Dor | 8 m .6 (B) | 11 m .5 (B) | 2.9 | S Doradus (SDOR) (Prototyp) | in der Großen Magellanschen Wolke | |||
| R Dra | Draco | 6 m .7 | 13 m .2 | 6,5 | 246 d | Mira-Variable (M) | ||
| T Eri | Eridanus | 7 m .2 | 13 m .2 | 6.0 | 252 d | Mira-Variable (M) | ||
| R für | Fornax | 7 m .5 | 13 m .0 | 5,5 | 389 d | Mira-Variable (M) | ||
| η Gem (Propus) | Zwillinge | 3 m .15 | 3 m .9 | 0,75 | 233 d | Semireguläre Form (SRA+EA) | ||
| ζ Gem (Mekbuda) | 3 m .62 | 4 m .18 | 0,56 | 10.15073 d | Klassischer Cepheiden (DCEP) | |||
| R Gem | Hind , 1848 | 6 m .0 | 14 m .0 | 8.0 | 370 d | Mira-Variable (M) | ||
| S Gem | Hind , 1848 | 8 m .0 | 14 m .7 | 6.7 | 293 d | Mira-Variable (M) | ||
| T Gem | Hind , 1848 | 8 m .0 | 15 m .0 | 7.0 | 288 d | Mira-Variable (M) | ||
| U Gem | 8 m .2 | 14 m .9 | 6.7 | (105.2 d) | Zwergnova (UGSS+E) | |||
| S Gru | Grus | 6 m .0 | 15 m .0 | 9.0 | 402 d | Mira-Variable (M) | ||
| α Her (Rasalgethi) | Herkules | William Herschel , 1759 | 2 m .74 | 4 m .0 | 1.26 | Halbregulär (SRC) | ||
| g Her (30 Her) | 4 m .3 | 6 m .3 | 2.0 | 89,2 d | Halbregulär (SRB) | |||
| u Her (68 Her) | 4 m .69 | 5 m .37 | 0,68 | 2.05103 d | Bedeckungsveränderlicher vom Algol-Typ (EA/SD) | |||
| S Her | 6 m .4 | 13 m .8 | 7.4 | 307 d | Mira-Variable (M) | |||
| U Her | 6 m .4 | 13 m .4 | 7.0 | 406 d | Mira-Variable (M) | |||
| X Her | 7 m .5 (p) | 8 m .6 (p) | 1.1 | 95,0 d | Halbregulär (SRB) | |||
| R Hor | Horologium | 4 m .7 | 14 m .3 | 9.6 | 408 d | Mira-Variable (M) | ||
| U Hor | 7 m .8 (p) | 15 m .1 (p) | 6.3 | 348 d | Mira-Variable (M) | |||
| R Hya | Hydra | Maraldi , 1704 | 3 m .5 | 10 m .9 | 7.4 | 389 d | Mira-Variable (M) | |
| S Hya | Hind , 1848 | 7 m .2 | 13 m .3 | 6.1 | 257 d | Mira-Variable (M) | ||
| U Hya | 7 m .0 (B) | 9 m .4 (B) | 2.4 | ~450 Tage | Halbregulär (SRB) | |||
| VW Hya | 10 m .5 | 14 m .1 | 3.6 | 2,69642 d | Bedeckungsveränderlicher vom Algol-Typ (EA/SD) | |||
| BL Lac | Lacerta | 12 m .4 (B) | 17 m .2 (B) | 4.8 | BLLAC-Prototyp | Ursprünglich hielt man ihn für einen veränderlichen Stern, aber später sich als Blazar herausstellte | ||
| R Leo | Löwe | JA Koch , 1782 | 4 m .4 | 11 m .3 | 6.9 | 310 d | Mira-Variable (M) | |
| R Lep | Lepus | 5 m .5 | 11 m .7 | 6.2 | 427 d | Mira-Variable (M) | Hinds Purpurstern | |
| RX Lep | 5 m .0 | 7 m .4 | 2.4 | ~60 Tage | Halbregulär (SRB) | |||
| R LMi | Leo Minor | 6 m .3 | 13 m .2 | 6.9 | 372 d | Mira-Variable (M) | ||
| RU Lup | Lupus | 9 m .6 (p) | 13 m .4 (p) | 3.8 | Orion-Variable (INT) | |||
| β Lyr (Sheliak) | Lyra | John Goodricke , 1784 | 3 m .25 | 4 m .36 | 1.11 | 12,91383 d | Bedeckungsveränderlicher vom Typ Beta Lyrae (Prototyp) | |
| R Lyr | 3 m .88 | 5 m .0 | 1.12 | ~46 Tage | Halbregulär (SRB) | |||
| RR Lyr | 7 m .06 | 8 m .12 | 1.06 | 0,566868 d | RR Lyrae Variable (Prototyp) | |||
| U Mic | Mikroskop | 7 m .0 | 14 m .4 | 7,7 | 334 d | Mira-Variable (M) | ||
| U Mon | Einhorn | 6 m .1 (p) | 8 m .8 (p) | 2.7 | 91,3 d | RV Tauri-Variable (RVB) | ||
| V Mon | 6 m .0 | 13 m .9 | 7.9 | 341 d | Mira-Variable (M) | |||
| R Nor | Norma | 6 m .5 (p) | 13 m .9 (p) | 7.4 | 508 d | Mira-Variable (M) | ||
| T Nor | 6 m .2 | 13 m .6 | 7.4 | 241 d | Mira-Variable (M) | |||
| R Okt. | Oktane | 6 m .4 | 13 m .2 | 6.8 | 405 d | Mira-Variable (M) | ||
| S Okt | 7 m .2 | 14 m .0 | 6.8 | 259 d | Mira-Variable (M) | |||
| V Oph | Schlangenträger | 7 m .3 | 11 m .6 | 4.3 | 297 d | Mira-Variable (M) | ||
| X Oph | 5 m .9 | 9 m .2 | 3.3 | 329 d | Mira-Variable (M) | |||
| RS Oph | 4 m .3 | 12 m .5 | 8.2 | recurrent nova (NR) | ||||
| BF Oph | 6 m .93 | 7 m .71 | 0,78 | 4,06775 d | Klassischer Cepheiden (DCEP) | |||
| α Ori ( Betelgeuse ) | Orion | John Herschel , 1840 | 0 m .0 | 1 m .3 | 1.3 | 6,39 Jahre | Halbregulär (SRC) | |
| δ Ori ( Mintaka ) | John Herschel , 1834 | 2 m .14 | 2 m .26 | 0,12 | 5,73248 d | Bedeckungsveränderlicher vom Algol-Typ (EA/DM) | ||
| R Ori | Hind , 1848 | 9 m .05 | 13 m .4 | 4,35 | 377 d | Mira-Variable (M) | ||
| U Ori | 4 m .8 | 13 m .0 | 8,5 | 368 d | Mira-Variable (M) | |||
| W Ori | 8 m .2 (p) | 12 m .4 (p) | 4.2 | 212 d | Halbregulär (SRB) | |||
| VV Ori | 5 m .31 | 5 m .66 | 0,35 | 1,48538 d | Verdunkelnder binärer Algol-Typ (EA/KE:) | |||
| CK Ori | 5 m .9 | 7 m .1 | 1.2 | ~120 Tage | Halbregulär (SR:) | |||
| κ Pav | Pavo | 3 m .91 | 4 m .78 | 0,87 | 9,09423 d | Cepheiden vom Typ II (CW) | ||
| S Pav | 6 m .6 | 10 m .4 | 3.8 | 381 d | Semireguläre (SRA) | |||
| β Peg (Scheat) | Pegasus | Schmidt , 1847 | 2 m .31 | 2 m .74 | 0,43 | LB | ||
| ε Peg (Enif) | 0 m .7 | 3 m .5 | 2.8 | LC | ||||
| R Peg | Hind , 1848 | 6 m .9 | 13 m .8 | 6.9 | 378 d | Mira-Variable (M) | ||
| X-Stift | 8 m .8 | 14 m .4 | 5.8 | 201 d | Mira-Variable (M) | |||
| β Per ( Algol ) | Perseus | Geminiano Montanari , 1669 | 2 m .12 | 3 m .39 | 1.27 | 2,86730 d | Bedeckungsveränderlicher vom Algol-Typ (EA/SD) (Prototyp) | Der Dämonenstern |
| DY Persei | R Coronae Borealis / DY Persei / (Prototyp) | |||||||
| φ Per (Dajiangjunbei) | 3 m .96 | 4 m .11 | 0,15 | 19,5 Tage | Gamma Cassiopeiae (GCAS) | |||
| ρ Per | 3 m .30 | 4 m .0 | 0,70 | ~50 Tage | Halbregulär (SRB) | |||
| X pro | 6 m .03 | 7 m .0 | 0,97 | Gamma Cassiopeiae (GCAS+XP) | ||||
| ζ Phe (Wurren) | Phönix | 3 m .91 | 4 m .42 | 0,51 | 1,66977 d | Bedeckungsveränderlicher vom Algol-Typ (EA/DM) | ||
| R Pic | Pictor | 6 m .35 | 10 m .1 | 3,75 | 171 d | Halbregulär (SR) | ||
| R Psc | Fische | Hind , 1850 | 7 m .0 | 14 m .8 | 7,8 | 345 d | Mira-Variable (M) | |
| TX Psc | 4 m .79 | 5 m .20 | 0,42 | LB | ||||
| L 2 Welpe | Welpen | 2 m .6 | 6 m .2 | 3.6 | 141 d | Halbregulär (SRB) | ||
| RS Welpe | 6 m .52 | 7 m .67 | 1.15 | 41.3876 d | Klassischer Cepheiden (DCEP) | |||
| T Pyx | Pyxis | 7 m .0 (B) | 15 m .77 (B) | 8,77 | (20 Jahre) | recurrent nova (NR) | ||
| S Scl | Bildhauer | 5 m .5 | 13 m .6 | 8.1 | 363 d | Mira-Variable (M) | ||
| RR Sco | Skorpion | 5 m .0 | 12 m .4 | 7.4 | 281 d | Mira-Variable (M) | ||
| RS Sco | 6 m .2 | 13 m .0 | 6.8 | 320 d | Mira-Variable (M) | |||
| RT Sco | 7 m .0 | 15 m .2 | 8.2 | 449 d | Mira-Variable (M) | |||
| R Sct | Scutum | Pigott , 1795 | 4 m .2 | 8 m .6 | 4.4 | 146,5 d | RV Tauri-Variable (RVA) | |
| R Ser | Serpens | Harding , 1826 | 5 m .16 | 14 m .4 | 9.24 | 356 d | Mira-Variable (M) | |
| S Ser | Harding , 1828 | 7 m .0 | 14 m .1 | 7.1 | 372 d | Mira-Variable (M) | ||
| U Sge | Sagitta | 6 m .45 | 9 m .28 | 2,83 | 3,38062 d | Bedeckungsveränderlicher vom Algol-Typ (EA/SD) | ||
| WZ Sge | 7 m .0 (B) | 15 m .53 (B) | 8,53 | (33 Jahre) | Zwergnova (UGSU+E+ZZ) | |||
| RR Sgr | Schütze | 5 m .4 | 14 m .0 | 8.6 | 336 d | Mira-Variable (M) | ||
| R Sgr | 6 m .7 | 12 m .83 | 6.13 | 270 d | Mira-Variable (M) | |||
| U Sgr | Schütze (im M25 ) | 6 m .28 | 7 m .15 | 0,87 | 6,74523 d | Klassischer Cepheiden (DCEP) | ||
| RT Sgr | Schütze | 6 m .0 | 14 m .1 | 8.1 | 306 d | Mira-Variable (M) | ||
| RU Sgr | 6 m .0 | 13 m .8 | 7,8 | 240 Tage | Mira-Variable (M) | |||
| RY Sgr | 5 m .8 | 14 m .0 | 8.2 | R Coronae Borealis (RCB) | ||||
| VX Sgr | 6 m .52 | 14 m .0 | 7.08 | 732 d | Halbregulär (SRC) | |||
| λ Tau | Stier | Baxendell , 1848 | 3 m .37 | 3 m .91 | 0,54 | 3,95295 d | Bedeckungsveränderlicher vom Algol-Typ (EA/DM) | |
| R Tau | Hind , 1849 | 7 m .6 | 15 m .8 | 8.2 | 321 d | Mira-Variable (M) | ||
| T Tau | 9 m .3 | 13 m .5 | 4.2 | Orion-Variable (INT) | ||||
| SU Tau | 9 m .1 | 16 m .86 | 7,76 | R Coronae Borealis (RCB) | ||||
| R Tri | Dreieck | 5 m .4 | 12 m .6 | 7.2 | 267 d | Mira-Variable (M) | ||
| R UMa | Großer Bär | 6 m .5 | 13 m .7 | 7.2 | 302 d | Mira-Variable (M) | ||
| T UMa | 6 m .6 | 13 m .5 | 6.9 | 257 d | Mira-Variable (M) | |||
| U UMa | 6 m .20 | 6 m .25 | 0,05 | - | ||||
| W UMa | 7 m .75 | 8 m .48 | 0,73 | 0,3336 d | Verfinsterndes Binärsystem vom Typ W Ursae Majoris (Prototyp) | |||
| Z UMa | 6 m .2 | 9 m .4 | 3.2 | 196 d | Halbregulär (SRB) | |||
| α UMi ( Polaris ) | Kleiner Bär | 1 m .86 | 2 m .13 | 0,27 | 3,9696 d | Klassischer Cepheiden (DCEPS) | ||
| R Vir | Jungfrau | Harding , 1809 | 6 m .1 | 12 m .1 | 6.0 | 146 d | Mira-Variable (M) | |
| S Vir | 6 m .3 | 13 m .2 | 6.9 | 375 d | Mira-Variable (M) |
Anmerkungen
- ^ Samus', NN; Kazarovets, EV; Durlevich, OV; Kireeva, NN; Pastukhova, EN (2017). „Gesamtkatalog veränderlicher Sterne: Version GCVS 5.1“. Astronomieberichte . 61 (1): 80. Bibcode : 2017ARep...61...80S . doi : 10.1134/S1063772917010085 .
- ^ (visuelle Größe, sofern nicht mit (B) (= blau) oder (p) (= fotografisch) gekennzeichnet)
- ^ (visuelle Größe, sofern nicht mit (B) (= blau) oder (p) (= fotografisch) gekennzeichnet)
Referenzen
- David H. Levy, Beobachtung veränderlicher Sterne: Ein Leitfaden für Anfänger
- Allgemeiner Katalog der veränderlichen Sterne
