Near-infrared observations of outflows and young stellar objects in the massive star-forming region AFGL 5180
Artikel i vetenskaplig tidskrift, 2024
Context. Massive stars play important roles throughout the universe; however, their formation remains poorly understood. Observations of jets and outflows in high-mass star-forming regions, as well as surveys of young stellar object (YSO) content, can help test theoretical models of massive star formation. Aims. We aim at characterizing the massive star-forming region AFGL 5180 in the near-infrared (NIR), identifying outflows and relating these to sub-mm/mm sources, as well as surveying the overall YSO surface number density to compare to massive star formation models. Methods. Broad- and narrow-band imaging of AFGL 5180 was made in the NIR with the Large Binocular Telescope, in both seeing-limited (~0.5′) and high angular resolution (~0.09′) Adaptive Optics (AO) modes, as well as with the Hubble Space Telescope. Archival continuum data from the Atacama Millimeter/Submillimeter Array (ALMA) was also utilized. Results. At least 40 jet knots were identified via NIR emission from H2 and [FeII] tracing shocked gas. Bright jet knots outflowing from the central most massive protostar, S4 (estimated mass ~11 M⊙, via SED fitting), are detected towards the east of the source and are resolved in fine detail with the AO imaging. Additional knots are distributed throughout the field, likely indicating the presence of multiple driving sources. Sub-millimeter sources detected by ALMA are shown to be grouped in two main complexes, AFGL 5180 M and a small cluster ~15′ (0.15 pc in projection) to the south, AFGL 5180 S. From our NIR continuum images we identify YSO candidates down to masses of ~0.1 M⊙. Combined with the sub-mm sources, this yields a surface number density of such YSOs of N* ~ 103pc-2 within a projected radius of about 0.1 pc. Such a value is similar to those predicted by models of both core accretion from a turbulent clump environment and competitive accretion. The radial profile of N* is relatively flat on scales out to 0.2 pc, with only modest enhancement around the massive protostar inside 0.05 pc, which provides additional constraints on these massive star formation models. Conclusions. This study demonstrates the utility of high-resolution NIR imaging, in particular with AO, for detecting outflow activity and YSOs in distant regions. The presented images reveal the complex morphology of outflow-shocked gas within the large-scale bipolar flow of a massive protostar, as well as clear evidence for several other outflow driving sources in the region. Finally, this work presents a novel approach to compare the observed YSO surface number density from our study against different models of massive star formation.
infrared: stars
techniques: high angular resolution
ISM: jets and outflows
stars: individual: AFGL 5180
stars: protostars
stars: formation
Författare
S. Crowe
University of Virginia
Consejo Superior de Investigaciones Científicas (CSIC)
R. Fedriani
Consejo Superior de Investigaciones Científicas (CSIC)
Jonathan Tan
University of Virginia
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
M. Whittle
University of Virginia
Y. Zhang
Shanghai Jiao Tong University
A. Caratti o. Garatti
Osservatorio Astronomico di Capodimonte
J. P. Farias
University of Texas
A. Gautam
University of Virginia
Z. Telkamp
University of Virginia
B. Rothberg
George Mason University
US Naval Observatory
M. Grudić
Carnegie Observatories
Morten Andersen
NOIRLab
Giuliana Cosentino
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
R. Garcia-Lopez
University College Dublin
Viviana Rosero
National Radio Astronomy Observatory
Kei E.I. Tanaka
Tokyo Institute of Technology
E. Pinna
ADaptive Optics National laboratory in Italy (ADONI)
Osservatorio Astrofisico di Arcetri
F. Rossi
Osservatorio Astrofisico di Arcetri
ADaptive Optics National laboratory in Italy (ADONI)
D. Miller
Large Binocular Telescope Observatory
G. Agapito
Osservatorio Astrofisico di Arcetri
ADaptive Optics National laboratory in Italy (ADONI)
C. Plantet
Osservatorio Astrofisico di Arcetri
ADaptive Optics National laboratory in Italy (ADONI)
E. Ghose
ADaptive Optics National laboratory in Italy (ADONI)
Osservatorio Astrofisico di Arcetri
J. Christou
Large Binocular Telescope Observatory
United States Gemini Office
J. Power
Large Binocular Telescope Observatory
A. Puglisi
Osservatorio Astrofisico di Arcetri
ADaptive Optics National laboratory in Italy (ADONI)
R. Briguglio
ADaptive Optics National laboratory in Italy (ADONI)
Osservatorio Astrofisico di Arcetri
G. Brusa
Large Binocular Telescope Observatory
G. Taylor
Large Binocular Telescope Observatory
X. Zhang
Large Binocular Telescope Observatory
T. Mazzoni
Osservatorio Astrofisico di Arcetri
ADaptive Optics National laboratory in Italy (ADONI)
M. Bonaglia
Osservatorio Astrofisico di Arcetri
ADaptive Optics National laboratory in Italy (ADONI)
S. Esposito
Osservatorio Astrofisico di Arcetri
ADaptive Optics National laboratory in Italy (ADONI)
C. Veillet
Large Binocular Telescope Observatory
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 682 A2Chockkompressioner i det interstellära mediet som triggers av Star Formation
Vetenskapsrådet (VR) (2021-05589), 2022-01-01 -- 2023-12-31.
Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
Fusion, plasma och rymdfysik
DOI
10.1051/0004-6361/202348094