The following is a list of stars with resolved images, that is,
stars whose images have been
resolved beyond a point source. Aside from the
Sun, observed from
Earth, stars are exceedingly small in apparent size, requiring the use of special high-resolution equipment and techniques to image. For example,
Betelgeuse, the first star other than the Sun to be directly imaged, has an angular diameter of only 50
milliarcseconds (mas).[1]
^Baron, F.; Monnier, J.; Pedretti, E.; Zhao, M.; Schaefer, G.; Parks, R.; Che, X.; Thureau, N.; ten Brummelaar, T. A.; McAlister, H. A.; Ridgway, S. T.; Farrington, C.; Sturmann, J.; Sturmann, L.; Turner, N. (2012). "Imaging the Algol Triple System in the H Band with the CHARA Interferometer". The Astrophysical Journal. 752 (1): 20.
arXiv:1205.0754.
Bibcode:
2012ApJ...752...20B.
doi:
10.1088/0004-637X/752/1/20.
S2CID11110989.
^Kővári, Zs.; Bartus, J.; Strassmeier, K. G.; Oláh, K.; Weber, M.; Rice, J. B.; Washuettl, A. (2007). "Doppler imaging of stellar surface structure. XXIII. The ellipsoidal K giant binary ζ Andromedae". Astronomy and Astrophysics. 463 (3): 1071.
arXiv:1301.0445.
Bibcode:
2007A&A...463.1071K.
doi:
10.1051/0004-6361:20065982.
^Roettenbacher, R.M.; Monnier, J.D.; Korhonen, H.; Aarnio, A.N.; Baron, F.; Che, X.; Harmon, R.O.; Kővári, Zs.; Kraus, S.; Schaefer, G.H.; Torres, G.; Zhao, M.; Ten Brummelaar, T.A.; Sturmann, J.; Sturmann, L. (2016). "No Sun-like dynamo on the active star ζ Andromedae from starspot asymmetry". Nature. 533 (7602): 217–220.
arXiv:1709.10107.
Bibcode:
2016Natur.533..217R.
doi:
10.1038/nature17444.
PMID27144357.
S2CID4466687.
^J.-B. Le Bouquin, S. Lacour, S. Renard, E. Thiébaut, A. Merand, T. Verhoelst, Pre-maximum spectro-imaging of the Mira star T Leporis with AMBER/VLTI, Astronomy and Astrophysics Volume 496, Number 1, March II 2009, L1–L4.
^Ohnaka, K; Hofmann, K.-H; Schertl, D; Weigelt, G; Baffa, C; Chelli, A; Petrov, R; Robbe-Dubois, S (2013). "High spectral resolution imaging of the dynamical atmosphere of the red supergiant Antares in the CO first overtone lines with VLTI/AMBER". Astronomy & Astrophysics. 555: A24.
arXiv:1304.4800.
Bibcode:
2013A&A...555A..24O.
doi:
10.1051/0004-6361/201321063.
S2CID56396587.
^Wittkowski, M; Abellan, F. J; Arroyo-Torres, B; Chiavassa, A; Guirado, J. C; Marcaide, J. M; Alberdi, A; De Wit, W. J; Hofmann, K.-H; Meilland, A; Millour, F; Mohamed, S; Sanchez-Bermudez, J (28 September 2017). "Multi-epoch VLTI-PIONIER imaging of the supergiant V766 Cen: Image of the close companion in front of the primary". Astronomy & Astrophysics. 1709: L1.
arXiv:1709.09430.
Bibcode:
2017A&A...606L...1W.
doi:
10.1051/0004-6361/201731569.
S2CID54740936.