Disruption of a massive molecular cloud by a supernova in the Galactic Centre: Initial results from the ACES project
Artikel i vetenskaplig tidskrift, 2024
The Milky Way's Central Molecular Zone (CMZ) differs dramatically from our local solar neighbourhood, both in the extreme interstellar medium conditions it exhibits (e.g. high gas, stellar, and feedback density) and in the strong dynamics at play (e.g. due to shear and gas influx along the bar). Consequently, it is likely that there are large-scale physical structures within the CMZ that cannot form elsewhere in the Milky Way. In this paper, we present new results from the Atacama Large Millimeter/submillimeter Array (ALMA) large programme ACES (ALMA CMZ Exploration Survey) and conduct a multi-wavelength and kinematic analysis to determine the origin of the M0.8-0.2 ring, a molecular cloud with a distinct ring-like morphology. We estimate the projected inner and outer radii of the M0.8-0.2 ring to be 79′′ and 154′′, respectively (3.1 pc and 6.1 pc at an assumed Galactic Centre distance of 8.2 kpc) and calculate a mean gas density >104 cm-3, a mass of ∼106 M⊙, and an expansion speed of ∼20 km s-1, resulting in a high estimated kinetic energy (>1051 erg) and momentum (>107 M⊙ km s-1). We discuss several possible causes for the existence and expansion of the structure, including stellar feedback and large-scale dynamics. We propose that the most likely cause of the M0.8-0.2 ring is a single high-energy hypernova explosion. To viably explain the observed morphology and kinematics, such an explosion would need to have taken place inside a dense, very massive molecular cloud, the remnants of which we now see as the M0.8-0.2 ring. In this case, the structure provides an extreme example of how supernovae can affect molecular clouds.
ISM: clouds
ISM: supernova remnants
Galaxy: center
ISM: bubbles
ISM: kinematics and dynamics
Författare
M. Nonhebel
University of St Andrews
European Southern Observatory (ESO)
Ashley T. Barnes
European Southern Observatory (ESO)
K. Immer
European Southern Observatory (ESO)
Jairo Armijos-Abendaño
Escuela Politécnica Nacional
Cardiff University
J. Bally
University of Colorado at Boulder
C. Battersby
University of Connecticut
M. G. Burton
Armagh Observatory and Planetarium
Natalie Butterfield
National Radio Astronomy Observatory
L. Colzi
Centro de Astrobiologia (CAB)
P. García
Universidad Catolica del Norte
Chinese Academy of Sciences
A. Ginsburg
College of Liberal Arts and Sciences
Jonathan D. Henshaw
Liverpool John Moores University
Max-Planck-Gesellschaft
Y. Hu
Institute for Advanced Studies
I. Jimenez-Serra
Centro de Astrobiologia (CAB)
R. S. Klessen
Universität Heidelberg
J.M. Diederik Kruijssen
Technische Universität München
COOL Research DAO
F. H. Liang
European Southern Observatory (ESO)
University of Oxford
S. Longmore
Liverpool John Moores University
X. Lu
Chinese Academy of Sciences
S. Martin
Atacama Large Millimeter-submillimeter Array (ALMA)
European Southern Observatory Santiago
E. A. C. Mills
University of Kansas
Francisco Nogueras-Lara
European Southern Observatory (ESO)
Maya Petkova
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
J. Pineda
Max-Planck-Gesellschaft
Consejo Superior de Investigaciones Científicas (CSIC)
Víctor M. Rivilla
Centro de Astrobiologia (CAB)
A. Sanchez-Monge
Centre Tecnològic de Telecomunicacions de Catalunya (CTTC)
Consejo Superior de Investigaciones Científicas (CSIC)
Max-Planck-Gesellschaft
Miriam G. Santa-Maria
College of Liberal Arts and Sciences
H. A. Smith
Harvard-Smithsonian Center for Astrophysics
Y. Sofue
University of Tokyo
Mattia C. Sormani
Universita degli Studi dell'Insubria
V. Tolls
Harvard-Smithsonian Center for Astrophysics
D. L. Walker
University of Manchester
J. Wallace
University of Connecticut
Q. D. Wang
University of Massachusetts
G. M. Williams
Aberystwyth University
Feng Wei Xu
Beijing University of Technology
Universität zu Köln
Astronomy and Astrophysics
0004-6361 (ISSN) 1432-0746 (eISSN)
Vol. 691 A70Opticon RadioNet Pilot
Europeiska kommissionen (EU) (EC/H2020/101004719), 2021-03-01 -- 2025-02-28.
Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
DOI
10.1051/0004-6361/202451190