Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FU Orionis

Discovery of an Accretion Streamer and a Slow Wide-angle Outflow around FU Orionis

We present Atacama Large Millimeter/submillimeter Array 12-m, 7-m, and Total Power Array observations of the FU Orionis outbursting system, covering spatial scales ranging from 160 to 25,000 au. The high-resolution interferometric data reveal an elongated ^12 CO(2–1) feature previously observed at l...

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Bibliographic Details
Main Authors: A. S. Hales, A. Gupta, D. Ruíz-Rodríguez, J. P. Williams, S. Pérez, L. Cieza, C. González-Ruilova, J. E. Pineda, A. Santamaría-Miranda, J. Tobin, P. Weber, Z. Zhu, A. Zurlo
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Star formation
FU Orionis stars
Young stellar objects
Online Access:https://doi.org/10.3847/1538-4357/ad31a1

Internet

https://doi.org/10.3847/1538-4357/ad31a1

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