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Cited article:

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A concordant scenario to explain FU Orionis from deep centimeter and millimeter interferometric observations

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Astronomy & Astrophysics 602 A19 (2017)
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ABSENCE OF SIGNIFICANT COOL DISKS IN YOUNG STELLAR OBJECTS EXHIBITING REPETITIVE OPTICAL OUTBURSTS

Hauyu Baobab Liu, Roberto Galván-Madrid, Eduard I. Vorobyov, Ágnes Kóspál, Luis F. Rodríguez, Michael M. Dunham, Naomi Hirano, Thomas Henning, Michihiro Takami, Ruobing Dong, Jun Hashimoto, Yasuhiro Hasegawa and Carlos Carrasco-González
The Astrophysical Journal Letters 816 (2) L29 (2016)
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CONFRONTING STANDARD MODELS OF PROTO-PLANETARY DISKS WITH NEW MID-INFRARED SIZES FROM THE KECK INTERFEROMETER

Rafael Millan-Gabet, Xiao Che, John D. Monnier, Michael L. Sitko, Ray W. Russell, Carol A. Grady, Amanda N. Day, R. B. Perry, Tim J. Harries, Alicia N. Aarnio, Mark M. Colavita, Peter L. Wizinowich, Sam Ragland and Julien Woillez
The Astrophysical Journal 826 (2) 120 (2016)
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THE PROGENITOR OF THE FUor-TYPE YOUNG ERUPTIVE STAR 2MASS J06593158–0405277

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The Astrophysical Journal 801 (1) L5 (2015)
https://doi.org/10.1088/2041-8205/801/1/L5

SPECTRAL ENERGY DISTRIBUTION ANALYSIS OF CLASS I AND CLASS II FU ORIONIS STARS

Luciana V. Gramajo, Javier A. Rodón and Mercedes Gómez
The Astronomical Journal 147 (6) 140 (2014)
https://doi.org/10.1088/0004-6256/147/6/140