Circumnuclear eccentric gas flow in the Galactic Center revealed by ALMA CMZ Exploration Survey (ACES)
Övrig text i vetenskaplig tidskrift, 2025
We analyze the CS ( J = 2-1 ) line cube from the internal data release obtained by the large-scale program "ALMA CMZ Exploration Survey ( ACES ) " to investigate the kinematic structure of the innermost similar to 10 pc region of the Galaxy, which contains the high-velocity compact cloud (HVCC) at (l, b, vLSR) similar to(+0 .degrees 02, -0 .degrees 02, 100 km s-1) ( hereafter G0.02 ) . The longitude-velocity diagram (LVD) of the cloud draws an elliptical structure, which is interpreted as an orbital trajectory in the (l, vLSR) space of a noncircular ( eccentric ) motion of the molecular gas in the gravitational potential of an extended mass distribution in the central 10 pc of the Galaxy. We argue that G0.02 is a kinematic tracer of the inner potential, a rare case of a dense an eccentric orbit in the nuclear field.
ISM: clouds
Galaxy: center
ISM: kinematics and dynamics
Galaxy: structure
ISM: molecules
Författare
Yoshiaki Sofue
University of Tokyo
Tomoharu Oka
Keio University
Steven N. Longmore
Liverpool John Moores University
Daniel Walker
University of Manchester
Adam Ginsburg
University of Florida
Jonathan D. Henshaw
Liverpool John Moores University
Max-Planck-Gesellschaft
John Bally
University of Colorado
Ashley T. Barnes
University of Colorado
Cara Battersby
University of Connecticut
Laura Colzi
Consejo Superior de Investigaciones Científicas (CSIC)
Paul Ho
National Taiwan University
Izaskun Jimenez-Serra
Consejo Superior de Investigaciones Científicas (CSIC)
Elizabeth Mills
University of Kansas
Maya Petkova
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Mattia C. Sormani
Universita degli Studi dell'Insubria
Jennifer Wallace
University of Connecticut
Jairo Armijos-Abendano
Escuela Politécnica Nacional
Katarzyna M. Dutkowska
Universiteit Leiden
Rei Enokiya
National Astronomical Observatory of Japan
Pablo Garcia
Chinese Academy of Sciences
Universidad Catolica del Norte
Savannah Gramze
University of Florida
Christian Henkel
Max-Planck-Gesellschaft
Yue Hu
Princeton University
Katharina Immer
University of Colorado
Yuhei Iwata
The Graduate University for Advanced Studies (SOKENDAI)
National Astronomical Observatory of Japan
Janik Karoly
University College London (UCL)
Ralf S. Klessen
Harvard University
Universität Heidelberg
Harvard-Smithsonian Center for Astrophysics
Kotaro Kohno
University of Tokyo
Mark R. Krumholz
Australian National University
Mark R. Morris
University of California
Jaime E. Pineda
Max-Planck-Gesellschaft
Sergio Martin
Atacama Large Millimeter-submillimeter Array (ALMA)
European Southern Observatory Santiago
Miguel Angel Requena-Torres
Towson University
Victor M. Rivilla
Consejo Superior de Investigaciones Científicas (CSIC)
Denise Riquelme-Vasquez
Universidad de La Serena
Alvaro Sanchez-Monge
Inst Estudis Espacials Catalunya IEEC
Universitat Autonoma de Barcelona (UAB)
Miriam G. Santa-Maria
University of Florida
Howard A. Smith
Harvard-Smithsonian Center for Astrophysics
Volker Tolls
Harvard-Smithsonian Center for Astrophysics
Q. Daniel Wang
University of Massachusetts
Publication of the Astronomical Society of Japan
0004-6264 (ISSN) 2053051x (eISSN)
Vol. 77 4 L55-L62Ämneskategorier (SSIF 2025)
Atom- och molekylfysik och optik
Astronomi, astrofysik och kosmologi
DOI
10.1093/pasj/psaf072