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 resolved, has an angular diameter of only 50 milliarcseconds (mas).[1]
↑Published 2024 based on observations from 2014 and 2020
↑First peer-reviewed publication in 2021, based on observations from 2011-2016
References
↑ 1.01.1H.Uitenbroek; Dupree, A. K.; Gilliland, R. L. (1998). "Spatially Resolved Hubble Space Telescope Spectra of the Chromosphere of alpha Orionis". Astronomical Journal116 (5): 2501. doi:10.1086/300596. Bibcode: 1998AJ....116.2501U.
↑Baron, F.; Monnier, J.; Pedretti, E.; Zhao, M.; Schaefer, G.; Parks, R.; Che, X.; Thureau, N. et al. (2012). "Imaging the Algol Triple System in the H Band with the CHARA Interferometer". The Astrophysical Journal752 (1): 20. doi:10.1088/0004-637X/752/1/20. Bibcode: 2012ApJ...752...20B.
↑ 7.07.17.2Gordon, Kathryn D.; Gies, Douglas R.; Schaefer, Gail H.; Huber, Daniel; Ireland, Michael (7 March 2019). "Angular Sizes, Radii, and Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal873 (1): 91. doi:10.3847/1538-4357/ab04b2. Bibcode: 2019ApJ...873...91G.
↑Roettenbacher, Rachael M.; Monnier, John D.; Korhonen, Heidi; Harmon, Robert O.; Baron, Fabien; Hackman, Thomas; Henry, Gregory W.; Schaefer, Gail H. et al. (2017-11-01). "Contemporaneous Imaging Comparisons of the Spotted Giant σ Geminorum Using Interferometric, Spectroscopic, and Photometric Data". The Astrophysical Journal849 (2): 120. doi:10.3847/1538-4357/aa8ef7. ISSN0004-637X. Bibcode: 2017ApJ...849..120R.
↑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 Astrophysics463 (3): 1071. doi:10.1051/0004-6361:20065982. Bibcode: 2007A&A...463.1071K.
↑Roettenbacher, R.M.; Monnier, J.D.; Korhonen, H.; Aarnio, A.N.; Baron, F.; Che, X.; Harmon, R.O.; Kővári, Zs. et al. (2016). "No Sun-like dynamo on the active star ζ Andromedae from starspot asymmetry". Nature533 (7602): 217–220. doi:10.1038/nature17444. PMID27144357. Bibcode: 2016Natur.533..217R.
↑ 12.012.1Woodruff, H. C.; Eberhardt, M.; Driebe, T.; Hofmann, K.-H. et al. (2004). "Interferometric observations of the Mira star o Ceti with the VLTI/VINCI instrument in the near-infrared". Astronomy & Astrophysics421 (2): 703–714. doi:10.1051/0004-6361:20035826. Bibcode: 2004A&A...421..703W.
↑Evans, Nancy Remage; Schaefer, Gail H.; Gallenne, Alexandre; Torres, Guillermo; Horch, Elliott P.; Anderson, Richard I.; Monnier, John D.; Roettenbacher, Rachael M. et al. (2024-08-01). "The Orbit and Dynamical Mass of Polaris: Observations with the CHARA Array". The Astrophysical Journal971 (2): 190. doi:10.3847/1538-4357/ad5e7a. ISSN0004-637X. Bibcode: 2024ApJ...971..190E.
↑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.
↑ 17.017.117.2Wallstrom, S. H. J.; Danilovich, T.; Muller, H. S. P.; Gottlieb, C. A.; Maes, S.; Van de Sande, M.; Decin, L.; Richards, A. M. S. et al. (December 6, 2023). "ATOMIUM: Molecular inventory of 17 oxygen-rich evolved stars observed with ALMA". Astronomy & Astrophysics681: A50. doi:10.1051/0004-6361/202347632. ISSN0004-6361.
↑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 & Astrophysics555: A24. doi:10.1051/0004-6361/201321063. Bibcode: 2013A&A...555A..24O.
↑Joyce, Meridith; Leung, Shing-Chi; Molnár, László; Ireland, Michael; Kobayashi, Chiaki; Nomoto, Ken’ichi (2020-10-01). "Standing on the Shoulders of Giants: New Mass and Distance Estimates for Betelgeuse through Combined Evolutionary, Asteroseismic, and Hydrodynamic Simulations with MESA". The Astrophysical Journal902 (1): 63. doi:10.3847/1538-4357/abb8db. ISSN0004-637X. Bibcode: 2020ApJ...902...63J.
↑M. Zhao (2008). "First Resolved Images Of The Eclipsing And Interacting Binary Beta Lyrae". The Astrophysical Journal684 (2): L95–L98. doi:10.1086/592146. Bibcode: 2008ApJ...684L..95Z.
↑ 30.030.130.2Kloppenborg, B. K.; Stencel, R. E.; Monnier, J. D.; Schaefer, G. H.; Baron, F.; Tycner, C.; Zavala, R. T.; Hutter, D. et al. (2015). "Interferometry of ɛ Aurigae: Characterization of the Asymmetric Eclipsing Disk". The Astrophysical Journal Supplement Series220 (1): 14. doi:10.1088/0067-0049/220/1/14. Bibcode: 2015ApJS..220...14K.
↑Bailer-Jones, C. A. L.; Rybizki, J.; Fouesneau, M.; Demleitner, M.; Andrae, R. (2021). "Estimating Distances from Parallaxes. V. Geometric and Photogeometric Distances to 1.47 Billion Stars in Gaia Early Data Release 3". The Astronomical Journal161 (3): 147. doi:10.3847/1538-3881/abd806. Bibcode: 2021AJ....161..147B.SU Persei's database entry at VizieR.
↑Anugu, Narsireddy; Gies, Douglas R.; Roettenbacher, Rachael M.; Monnier, John D.; Montargés, Miguel; Mérand, Antoine; Baron, Fabien; Schaefer, Gail H. et al. (September 2024). "Time Evolution Images of the Hypergiant RW Cephei during the Rebrightening Phase Following the Great Dimming" (in en). The Astrophysical Journal Letters973 (1): L5. doi:10.3847/2041-8213/ad736c. ISSN2041-8205. Bibcode: 2024ApJ...973L...5A.
↑Anugu, Narsireddy; Baron, Fabien; Gies, Douglas R.; Lanthermann, Cyprien; Schaefer, Gail H.; Shepard, Katherine A.; ten Brummelaar, Theo; Monnier, John D. et al. (July 2023). "The Great Dimming of the hypergiant star RW Cephei: CHARA Array images and spectral analysis". The Astronomical Journal166 (2): 78. doi:10.3847/1538-3881/ace59d. Bibcode: 2023AJ....166...78A.
↑Wittkowski, M; Abellan, F. J; Arroyo-Torres, B; Chiavassa, A; Guirado, J. C; Marcaide, J. M; Alberdi, A; De Wit, W. J et al. (28 September 2017). "Multi-epoch VLTI-PIONIER imaging of the supergiant V766 Cen: Image of the close companion in front of the primary". Astronomy & Astrophysics1709: L1. doi:10.1051/0004-6361/201731569. Bibcode: 2017A&A...606L...1W.
↑Munoz-Sanchez, G.; Kalitsounaki, M.; Wit, S. de; Antoniadis, K.; Bonanos, A. Z.; Zapartas, E.; Boutsia, K.; Christodoulou, E. et al. (2024-12-02), The dramatic transition of the extreme Red Supergiant WOH G64 to a Yellow Hypergiant