WEAVE First Light Observations: Origin and Dynamics of the Shock Front in Stephan's Quintet
Journal article, 2024
We present a detailed study of the large-scale shock front in Stephan's Quintet, a by-product of past and ongoing interactions. Using integral-field spectroscopy from the new William Herschel Telescope Enhanced Area Velocity Explorer (WEAVE), recent 144 MHz observations from the LOFAR Two-metre Sky Survey, and archival data from the Very Large Array and JWST, we obtain new measurements of key shock properties and determine its impact on the system. Harnessing the WEAVE large integral field unit's field of view (90 x 78 arcsec(2)), spectral resolution (R similar to 2500), and continuous wavelength coverage across the optical band, we perform robust emission-line modelling and dynamically locate the shock within the multiphase intergalactic medium with higher precision than previously possible. The shocking of the cold gas phase is hypersonic, and comparisons with shock models show that it can readily account for the observed emission-line ratios. In contrast, we demonstrate that the shock is relatively weak in the hot plasma visible in X-rays (with Mach number of M similar to 2-4), making it inefficient at producing the relativistic particles needed to explain the observed synchrotron emission. Instead, we propose that it has led to an adiabatic compression of the medium, which has increased the radio luminosity 10-fold. Comparison of the Balmer line-derived extinction map with the molecular gas and hot dust observed with JWST suggests that pre-existing dust may have survived the collision, allowing the condensation of H-2 - a key channel for dissipating the shock energy.
galaxies: interactions
techniques: imaging spectroscopy
radio continuum: ISM
galaxies: groups: individual: Stephan's Quintet
Author
Arnaudova
University of Hertfordshire
S. Das
University of Hertfordshire
D. J. B. Smith
University of Hertfordshire
M. J. Hardcastle
University of Hertfordshire
N. Hatch
University of Nottingham
S. C. Trager
University of Groningen
R. J. Smith
Durham University
A. B. Drake
University of Hertfordshire
J. C. McGarry
University of Hertfordshire
S. Shenoy
University of Hertfordshire
J. P. Stott
Lancaster University
J. H. Knapen
Instituto de Astrofísica de Canarias
University of La Laguna
Kelley Michelle Hess
Chalmers, Space, Earth and Environment, Onsala Space Observatory
K. J. Duncan
University of Edinburgh
A. Gloudemans
NSF's National Optical-Infrared Astronomy Research Laboratory (NOIRLab)
P. N. Best
University of Edinburgh
R. Garcia-Benito
Spanish National Research Council (CSIC)
R. Kondapally
University of Edinburgh
M. Balcells
University of La Laguna
Instituto de Astrofísica de Canarias
Isaac Newton Grp Telescopes
G. S. Couto
Leibniz Association
D. C. Abrams
Isaac Newton Grp Telescopes
D. Aguado
University of La Laguna
Instituto de Astrofísica de Canarias
J. A. L. Aguerri
University of La Laguna
Instituto de Astrofísica de Canarias
R. Barrena
University of La Laguna
Instituto de Astrofísica de Canarias
C. R. Benn
Isaac Newton Grp Telescopes
T. Bensby
Lund University
S. R. Berlanas
Instituto de Astrofísica de Canarias
University of La Laguna
D. Bettoni
Istituto nazionale di astrofisica (INAF)
D. Cano-Infantes
Isaac Newton Grp Telescopes
R. Carrera
Istituto nazionale di astrofisica (INAF)
P. J. Concepcion
Isaac Newton Grp Telescopes
G. B. Dalton
Science and Technology Facilities Council (STFC)
University of Oxford
G. D'Ago
University of Cambridge
K. Dee
Isaac Newton Grp Telescopes
L. Dominguez-Palmero
Isaac Newton Grp Telescopes
University of La Laguna
Instituto de Astrofísica de Canarias
J. E. Drew
University College London (UCL)
E. L. Escott
Durham University
C. Farina
University of La Laguna
Instituto de Astrofísica de Canarias
Isaac Newton Grp Telescopes
M. Fossati
University of Milano-Bicocca
Istituto nazionale di astrofisica (INAF)
M. Fumagalli
Istituto nazionale di astrofisica (INAF)
University of Milano-Bicocca
E. Gafton
Isaac Newton Grp Telescopes
F. J. Gribbin
Isaac Newton Grp Telescopes
S. Hughes
University of Cambridge
A. Iovino
Istituto nazionale di astrofisica (INAF)
S. Jin
University of Groningen
I. J. Lewis
University of Oxford
M. Longhetti
Istituto nazionale di astrofisica (INAF)
J. Mendez-Abreu
University of La Laguna
Instituto de Astrofísica de Canarias
A. Mercurio
Istituto nazionale di astrofisica (INAF)
University of Salerno
A. Molaeinezhad
University of Cambridge
E. Molinari
Istituto nazionale di astrofisica (INAF)
M. Monguio
University of Barcelona
Dribia Data Research
D. N. A. Murphy
University of Cambridge
S. Pico
Isaac Newton Grp Telescopes
M. M. Pieri
Aix Marseille University
A. W. Ridings
Isaac Newton Grp Telescopes
M. Romero-Gomez
Centre Tecnològic de Telecomunicacions de Catalunya (CTTC)
University of Barcelona
E. Schallig
University of Oxford
T. W. Shimwell
Netherlands Institute for Radio Astronomy (ASTRON)
Leiden University
J. Skvarc
Isaac Newton Grp Telescopes
R. Stuik
NOVA
Leiden University
A. Vallenari
Istituto nazionale di astrofisica (INAF)
J. M. van der Hulst
University of Groningen
N. A. Walton
University of Cambridge
C. C. Worley
University of Cambridge
University of Canterbury
Monthly Notices of the Royal Astronomical Society
0035-8711 (ISSN) 1365-2966 (eISSN)
Vol. 535 3 2269-2290Subject Categories (SSIF 2011)
Astronomy, Astrophysics and Cosmology
DOI
10.1093/mnras/stae2235
Related datasets
URI: http://portal.was.tng.iac.es/