English

Variations in the $\Sigma_{\rm SFR} {-} \Sigma_{\rm mol} {-} \Sigma_{\rm \star}$ plane across galactic environments in PHANGS galaxies

Astrophysics of Galaxies 2022-07-13 v3

Abstract

There exists some consensus that stellar mass surface density (Σ\Sigma_{*}) and molecular gas mass surface density (Σmol\Sigma_{\rm mol}) are the main quantities responsible for locally setting the star formation rate. This regulation is inferred from locally resolved scaling relations between these two quantities and the star formation rate surface density (ΣSFR\Sigma_{\rm SFR}). However, the universality of these relations is debated. Here, we probe the interplay between these three quantities across different galactic environments at a spatial resolution of 150 pc. We perform a hierarchical Bayesian linear regression to find the best set of parameters CC_{*}, CmolC_{\rm mol}, and CnormC_{\rm norm} that describe the star-forming plane conformed by these quantities, such that logΣSFR=ClogΣ+CmollogΣmol+Cnorm\log \Sigma_{\rm SFR} = C_{*} \log \Sigma_{*} + C_{\rm mol} \log \Sigma_{\rm mol} + C_{\rm norm}, and explore variations in the determined parameters across galactic environments, focusing our analysis on the CC_{*} and CmolC_{\rm mol} slopes. We find signs of variations in the posterior distributions of CC_{*} and CmolC_{\rm mol} across different galactic environments. Bars show the most negative value of CC_{*}, a sign of longer depletion times, while spiral arms show the highest CC_{*} among all environments. We conclude that systematic variations in the interplay of Σ\Sigma_{*}, Σmol\Sigma_{\rm mol} and ΣSFR\Sigma_{\rm SFR} across galactic environments exist at a spatial resolution of 150 pc, and we interpret these variations as produced by an additional mechanism regulating the formation of stars that is not captured by either Σ\Sigma_{*} or Σmol\Sigma_{\rm mol}. We find that these variations correlate with changes in the star formation efficiency across environments, which could be linked to the dynamical state of the gas that prevents it from collapsing and forming stars, or to changes in the molecular gas fraction.

Keywords

Cite

@article{arxiv.2203.11971,
  title  = {Variations in the $\Sigma_{\rm SFR} {-} \Sigma_{\rm mol} {-} \Sigma_{\rm \star}$ plane across galactic environments in PHANGS galaxies},
  author = {I. Pessa and E. Schinnerer and A. Leroy and E. Koch and E. Rosolowsky and T. Williams and H. -A. Pan and A. Schruba and A. Usero and F. Belfiore and F. Bigiel and G. Blanc and M. Chevance and D. Dale and E. Emsellem and J. Gensior and S. Glover and K. Grasha and B. Groves and R. Klessen and K. Kreckel and J. M. D. Kruijssen and D. Liu and S. E. Meidt and J. Pety and M. Querejeta and T. Saito and P. Sanchez-Blazquez and E. J. Watkins},
  journal= {arXiv preprint arXiv:2203.11971},
  year   = {2022}
}

Comments

21 pages, 16 figures, accepted for publication in A&A