|
|
[]
| , R☉ |
||
|---|---|---|
| № | ||
| 1 | VY | 18002100[1] |
| 2 | WOH G64 | 1738 [2] |
| 3 | VV A | 16001900 |
| 4 | V354 | 1520 |
| 5 | KW | 1460 |
| 6 | KY | 1420 |
| 7 | μ (« » ) | 1420 |
| 8 | (α ) | ~1000 |
| 9 | V509 | 910 |
| 10 | V838 | 800 |
| 11 | V382 | 747 |
| 12 | (α ) | 700[3] |
| 13 | S | 580[4] |
| 14 | S | 550 |
| 15 | T | 540[5] |
| 16 | S | 530[6] |
| 17 | W | 520[7] |
| 18 | 119 | 510[8] |
| 19 | R | 500[9] |
| 20 | (δ ) | 482 |
| 21 | χ | 470[10] |
| 22 | (α ) | 460 |
| 23 | ρ | 450 |
| 24 | A (ο ) | 400[11] |
| 25 | η | 400 |
| 26 | R | 370 |
| 27 | HR | 350 |
| 28 | R | 350[12] |
| 29 | 340 | |
| 30 | La Superba (Y Canum Venaticorum) | 300 |
| 31 | (α ) | 220 |
| 32 | LBV 1806-20 | 200 |
| 33 | ε A | 175 |
| 34 | I (ζ ) | 160[13] |
| 35 | (ε ) | 150 |
| 36 | (γ ) | 113 |
| 37 | (β ) A1 | 109 |
| 38 | (γ ) | 83 |
| 39 | (α ) | 77 |
| 40 | (β ) | 70 |
| 41 | (ε ) | 70 |
| 42 | R | 65 |
| 43 | (α ) | 65 |
| 44 | (δ ) | 60 |
| 45 | (ζ ) | 60 |
| 46 | (α ) | 60 |
| 47 | (ζ ) | 60 |
| 48 | η | 60 |
| 49 | (γ ) | 50 |
| 50 | (α ) | 43[14] |
| 51 | (β ) | 41 |
[] .
[]
- Roberta M. Humphreys VY Canis Majoris: The Astrophysical Basis of Its Luminosity (.) (pdf). 12 2009.
- K. Ohnaka, et al. Spatially resolved dusty torus toward the red supergiant WOH G64 in the Large Magellanic Cloud. Table 3 page 7 «derived from our radiative transfer modeling.»
- Catalogue of Stellar Diameters (CADARS) (ALF SCO) (.). 12 2012. 12 2009.
- Catalogue of Stellar Diameters (CADARS) (S PEG) (.). 12 2012. 12 2009.
- Catalogue of Stellar Diameters (CADARS) (T CEP) (.). 12 2012. 12 2009.
- Catalogue of Stellar Diameters (CADARS) (S ORI) (.). 12 2012. 12 2009.
- Catalogue of Stellar Diameters (CADARS) (W HYA) (.). 12 2012. 12 2009.
- Catalogue of Stellar Diameters (CADARS) (119 TAU) (.). 12 2012. 12 2009.
- Catalogue of Stellar Diameters (CADARS) (R CAS) (.). 12 2012. 12 2009.
- Catalogue of Stellar Diameters (CADARS) (KHI CYG) (.). 12 2012. 12 2009.
- H.C.Woodrua, M. Eberhardta, T. Driebe . Interferometric observations of the Mira star o Ceti with the VLTI/VINCI instrument in the near-infrared (.) (pdf). 12 2012. 12 2009.
- D. Fedele, M. Wittkowski, F. Paresce, M. Scholz, P.R. Wood, S. Ciroi The K-band intensity profile of R Leonis probed by VLTI/VINC (.). 12 2009.
- Catalogue of Stellar Diameters (CADARS) (ZET AUR) (.). 12 2012. 12 2009.
- Richichi, A.; Roccatagliata, V. Aldebaran's angular diameter: How well do we know it? (.). 12 2012. 12 2009.
[]
- Lowell Observatory Astronomers Identify Largest Stars Known
- BBC News Three largest stars identified
- 26
- 300
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