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: massive
Stars: individual: S255IR NIRS3
ISM: jets and outflows
Techniques: high angular resolution
Stars: pre-main sequence
ISM: kinematics and dynamics
Author
Rubén Fedriani
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
Institute of Astrophysics of Andalusia (IAA)
A. Caratti o. Garatti
Osservatorio Astronomico di Capodimonte
R. Cesaroni
Arcetri Astrophysical Observatory
Jonathan Tan
University of Virginia
Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics
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)
Vol. 676 A107Eld ur is - den massiva stjärnbildningens utvecklingsstadier
Swedish Research Council (VR) (2017-04522), 2018-01-01 -- 2021-12-31.
Shock Compressions in the Interstellar Medium as triggers of Star Formation
Swedish Research Council (VR) (2021-05589), 2022-01-01 -- 2023-12-31.
Star formation history of MAssive pRoTostars (SMART)
European Commission (EC) (EC/H2020/101032092), 2021-04-01 -- 2023-03-31.
Subject Categories
Subatomic Physics
Meteorology and Atmospheric Sciences
Astronomy, Astrophysics and Cosmology
DOI
10.1051/0004-6361/202346736