The bar-driven central complex of NGC 6946: A panchromatic and spatially resolved view of its star formation history and interstellar medium
Abstract
We present a multi-wavelength analysis of the nearby spiral galaxy NGC 6946, combining optical IFS, infrared, and radio observations. We aim to characterise both the integrated and spatially resolved properties of the stellar populations and ISM, and to interpret them in the context of bar-driven galaxy evolution. We used the SED fitting code SINOPSIS to derive stellar population properties, and different prescriptions to derive ISM properties including atomic and molecular gas masses and the dust mass,temperature, and emissivity index. We find that the central 2.6 kpc hosts 40% of the stellar mass, as well as the bulk of the molecular gas and dust, and has sustained enhanced star formation over cosmic time. A major star formation episode occurred 0.6 Gyr ago. The spatially resolved KS relation shows that molecular gas alone explains only part of the current SFR variance, while alternative prescriptions incorporating stellar mass and dynamical equilibrium pressure yield only modest improvements. We also find radial enhancements in the effective oxygen yield and gas mass fraction relative to surrounding regions, consistent with sustained gas accumulation. Together with the molecular gas streaming motions previously detected kinematic studies, our results are consistent with, and provide independent support for, the inward transport of gas driven by a system of nested bars and with a scenario in which a recent episode of bar-driven gas inflow enhanced the central molecular gas reservoir and sustained elevated star formation. These findings point to efficient HI-to-H2 conversion, likely promoted by the combined effect of the secondary bar and the large dust content, ultimately regulating star formation. We also find indications consistent with a young stellar bar. The current decline in star formation despite large gas reservoirs suggests recent bar-driven quenching.
Versions
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BibTeX
@misc{alvarezcordoba2026bardriven,
title = {{The bar-driven central complex of NGC 6946: A panchromatic and spatially resolved view of its star formation history and interstellar medium}},
author = {Santiago Álvarez-Córdoba and Jacopo Fritz and M. A. Lara-López and Bernardo Cervantes Sodi and L. S. Pilyugin and Viviana Casasola and Sami Dib and Omar López-Cruz and L. E. Garduño and G. Valé and I. A. Zinchenko and M. E. De Rossi and M. M. Puebla and Vidhi Tailor and Gustavo Bruzual and J. Zaragoza-Cardiel and Margarita Rosado},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.22483},
eprint = {2610.22483},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.22483},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - The bar-driven central complex of NGC 6946: A panchromatic and spatially resolved view of its star formation history and interstellar medium
AU - Santiago Álvarez-Córdoba
AU - Jacopo Fritz
AU - M. A. Lara-López
AU - Bernardo Cervantes Sodi
AU - L. S. Pilyugin
AU - Viviana Casasola
AU - Sami Dib
AU - Omar López-Cruz
AU - L. E. Garduño
AU - G. Valé
AU - I. A. Zinchenko
AU - M. E. De Rossi
AU - M. M. Puebla
AU - Vidhi Tailor
AU - Gustavo Bruzual
AU - J. Zaragoza-Cardiel
AU - Margarita Rosado
PY - 2026
DA - 2026/10/15
PB - arXiv
DO - 10.48550/arxiv.2610.22483
UR - https://arxiv.org/abs/2610.22483
AB - We present a multi-wavelength analysis of the nearby spiral galaxy NGC 6946, combining optical IFS, infrared, and radio observations. We aim to characterise both the integrated and spatially resolved properties of the stellar populations and ISM, and to interpret them in the context of bar-driven galaxy evolution. We used the SED fitting code SINOPSIS to derive stellar population properties, and different prescriptions to derive ISM properties including atomic and molecular gas masses and the dust mass,temperature, and emissivity index. We find that the central 2.6 kpc hosts 40% of the stellar mass, as well as the bulk of the molecular gas and dust, and has sustained enhanced star formation over cosmic time. A major star formation episode occurred 0.6 Gyr ago. The spatially resolved KS relation shows that molecular gas alone explains only part of the current SFR variance, while alternative prescriptions incorporating stellar mass and dynamical equilibrium pressure yield only modest improvements. We also find radial enhancements in the effective oxygen yield and gas mass fraction relative to surrounding regions, consistent with sustained gas accumulation. Together with the molecular gas streaming motions previously detected kinematic studies, our results are consistent with, and provide independent support for, the inward transport of gas driven by a system of nested bars and with a scenario in which a recent episode of bar-driven gas inflow enhanced the central molecular gas reservoir and sustained elevated star formation. These findings point to efficient HI-to-H_2 conversion, likely promoted by the combined effect of the secondary bar and the large dust content, ultimately regulating star formation. We also find indications consistent with a young stellar bar. The current decline in star formation despite large gas reservoirs suggests recent bar-driven quenching.
ER -