The sharpest view on the high-mass star-forming region S255IR: Near infrared adaptive optics imaging of the outbursting source NIRS3
Journal article, 2023
Stars: individual: S255IR NIRS3
Techniques: high angular resolution
Stars: massive
Stars: pre-main sequence
ISM: kinematics and dynamics
ISM: jets and outflows
Author
Rubén Fedriani
Spanish National Research Council (CSIC)
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
A. Caratti o. Garatti
Osservatorio Astronomico di Capodimonte
R. Cesaroni
Arcetri Astrophysical Observatory
Jonathan Tan
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
University of Virginia
B. Stecklum
Thüringer Landessternwarte Tautenburg
L. Moscadelli
Arcetri Astrophysical Observatory
M. Koutoulaki
University of Leeds
Giuliana Cosentino
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
M. Whittle
University of Virginia
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
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European Commission (EC) (EC/H2020/101032092), 2021-04-01 -- 2023-03-31.
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Swedish Research Council (VR) (2017-04522), 2018-01-01 -- 2021-12-31.
Subject Categories (SSIF 2011)
Subatomic Physics
Meteorology and Atmospheric Sciences
Astronomy, Astrophysics and Cosmology
DOI
10.1051/0004-6361/202346736