The impact of spiral arms on the star formation life cycle

Fuente: arXiv
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Main Authors: Romanelli, Andrea, Chevance, Mélanie, Kruijssen, J. M. Diederik, Ramambason, Lise, Querejeta, Miguel, Boquien, Mederic, Dale, Daniel A., Brok, Jakob den, Glover, Simon C. O., Grasha, Kathryn, Hughes, Annie, Kim, Jaeyeon, Longmore, Steven, Meidt, Sharon E., Mendez-Delgado, José Eduardo, Neumann, Lukas, Pety, Jérôme, Schinnerer, Eva, Smith, Rowan, Sun, Jiayi, Williams, Thomas G.
Format: Preprint
Published: 2025
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author Romanelli, Andrea
Chevance, Mélanie
Kruijssen, J. M. Diederik
Ramambason, Lise
Querejeta, Miguel
Boquien, Mederic
Dale, Daniel A.
Brok, Jakob den
Glover, Simon C. O.
Grasha, Kathryn
Hughes, Annie
Kim, Jaeyeon
Longmore, Steven
Meidt, Sharon E.
Mendez-Delgado, José Eduardo
Neumann, Lukas
Pety, Jérôme
Schinnerer, Eva
Smith, Rowan
Sun, Jiayi
Williams, Thomas G.
author_facet Romanelli, Andrea
Chevance, Mélanie
Kruijssen, J. M. Diederik
Ramambason, Lise
Querejeta, Miguel
Boquien, Mederic
Dale, Daniel A.
Brok, Jakob den
Glover, Simon C. O.
Grasha, Kathryn
Hughes, Annie
Kim, Jaeyeon
Longmore, Steven
Meidt, Sharon E.
Mendez-Delgado, José Eduardo
Neumann, Lukas
Pety, Jérôme
Schinnerer, Eva
Smith, Rowan
Sun, Jiayi
Williams, Thomas G.
contents 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 paper, we investigate 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 measure 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.
format Preprint
id arxiv_https___arxiv_org_abs_2505_10908
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle The impact of spiral arms on the star formation life cycle
Romanelli, Andrea
Chevance, Mélanie
Kruijssen, J. M. Diederik
Ramambason, Lise
Querejeta, Miguel
Boquien, Mederic
Dale, Daniel A.
Brok, Jakob den
Glover, Simon C. O.
Grasha, Kathryn
Hughes, Annie
Kim, Jaeyeon
Longmore, Steven
Meidt, Sharon E.
Mendez-Delgado, José Eduardo
Neumann, Lukas
Pety, Jérôme
Schinnerer, Eva
Smith, Rowan
Sun, Jiayi
Williams, Thomas G.
Astrophysics of Galaxies
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 paper, we investigate 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 measure 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.
title The impact of spiral arms on the star formation life cycle
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2505.10908