The impact of spiral arms on the star formation life cycle

The matter cycle between gas clouds and stars in galaxies plays a crucial role in regulating galaxy evolution through feedback mechanisms. In turn, the local and global galactic environments shape the interstellar medium and provide the initial conditions for star formation, potentially affecting the properties of this small-scale matter cycle. In particular, spiral arms have been proposed to play a pivotal role in the star formation life cycle, by enhancing the gas density and triggering star formation. However, their exact role is still debated. In this study, we investigated the role of spiral arms in the giant molecular cloud evolutionary life cycle and on the star formation process in a sample of 22 nearby spiral galaxies from the PHANGS survey. We measured the cloud lifetime, the feedback timescale, the typical distance between independent regions, and the star formation efficiency in spiral arms and inter-arm regions separately. We find that the distributions of the cloud lifetime as well as the feedback timescale are similar in both environments. This result suggests that spiral arms are unlikely to play a dominant role in triggering star formation. By contrast, the star formation efficiency appears to be slightly higher in inter-arm regions compared to spiral arms.

Authors

Publication Details

Journal
Astronomy and Astrophysics
Published
2025-05-15
DOI
https://doi.org/10.1051/0004-6361/202553895
Citations
2
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
2.31
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article

The impact of spiral arms on the star formation life cycle

M. Boquien, Sharon E. Meidt, Jaeyeon Kim, J. Pety et al.
2 citations
Astronomy and Astrophysics
Astro and Planetary Science
2.31
article

The impact of spiral arms on the star formation life cycle

M. Boquien, Sharon E. Meidt, Jaeyeon Kim, J. Pety, Mélanie Chevance, Lise Ramambason, J. Eduardo Méndez-Delgado, Miguel Querejeta, Lukas Neumann, Jakob S. den Brok, J. M. Diederik Kruijssen, Thomas G. Williams, Annie Hughes, Kathryn Grasha, Simon C. O. Glover, Eva Schinnerer, Jiayi Sun, Steven N. Longmore, Daniel A. Dale, Rowan J. Smith, Andrea Romanelli
article en
2 citations

Abstract

The matter cycle between gas clouds and stars in galaxies plays a crucial role in regulating galaxy evolution through feedback mechanisms. In turn, the local and global galactic environments shape the interstellar medium and provide the initial conditions for star formation, potentially affecting the properties of this small-scale matter cycle. In particular, spiral arms have been proposed to play a pivotal role in the star formation life cycle, by enhancing the gas density and triggering star formation. However, their exact role is still debated. In this study, we investigated the role of spiral arms in the giant molecular cloud evolutionary life cycle and on the star formation process in a sample of 22 nearby spiral galaxies from the PHANGS survey. We measured the cloud lifetime, the feedback timescale, the typical distance between independent regions, and the star formation efficiency in spiral arms and inter-arm regions separately. We find that the distributions of the cloud lifetime as well as the feedback timescale are similar in both environments. This result suggests that spiral arms are unlikely to play a dominant role in triggering star formation. By contrast, the star formation efficiency appears to be slightly higher in inter-arm regions compared to spiral arms.

Astronomy and AstrophysicsVol. 698
Openalex Percentile: Top 12%
Astro and Planetary Science
2.31
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