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

2017/01/23 by Hauyu Baobab Liu, Eduard I. Vorobyov, Ruobing Dong +17 · 35 citations
Chemistry · Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Bolometer #Galaxy #Luminosity #Millimeter #Molecular Spectroscopy and Structure #Optics #Physics #Spectral index #Spectral line #Stars #Stellar, planetary, and galactic studies #astro-ph.GA #astro-ph.SR

paper · pdf · doi:10.1051/0004-6361/201630263

published in Astronomy and Astrophysics 602, A19 (EDP Sciences) · 10 pages, 4 figures, referee reported received and replied

arxiv created 2017/01/23 · openalex publication_date 2017/02/21 · arxiv updated 2017/05/24 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims. The aim of this work is to constrain properties of the disk around the archetype FU Orionis object, FU Ori, with as good as ~25 au resolution.

Citations

• The Submillimeter Array
• Encounter-driven accretion in young stellar clusters – A connection to FUors?
• TIDALLY INDUCED BROWN DWARF AND PLANET FORMATION IN CIRCUMSTELLAR DISKS
• Constraints on photoevaporation models from (lack of) radio emission in the Corona Australis protoplanetary disks
• COLD CO GAS IN THE DISK OF THE YOUNG ERUPTIVE STAR EX LUP

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