Comparing the pre-SNe feedback and environmental pressures for 6000 H II regions across 19 nearby spiral galaxies

Article


Barnes, A. T., Glover, S. C. O., Kreckel, K., Ostriker, E. C., Bigiel, F., Belfiore, F., Bešlić, I., Blanc, G. A., Chevance, M., Dale, D. A., Egorov, O., Eibensteiner, C., Emsellem, E., Grasha, K., Groves, B. A., Klessen, R. S., Kruijssen, J. M. D., Leroy, A. K., Longmore, S. N., ..., Williams, T. G.. 2021. "Comparing the pre-SNe feedback and environmental pressures for 6000 H II regions across 19 nearby spiral galaxies." Monthly Notices of the Royal Astronomical Society. 508 (4), pp. 5362-5389. https://doi.org/10.1093/mnras/stab2958
Article Title

Comparing the pre-SNe feedback and environmental pressures for 6000 H II regions across 19 nearby spiral galaxies

ERA Journal ID1074
Article CategoryArticle
AuthorsBarnes, A. T., Glover, S. C. O., Kreckel, K., Ostriker, E. C., Bigiel, F., Belfiore, F., Bešlić, I., Blanc, G. A., Chevance, M., Dale, D. A., Egorov, O., Eibensteiner, C., Emsellem, E., Grasha, K., Groves, B. A., Klessen, R. S., Kruijssen, J. M. D., Leroy, A. K., Longmore, S. N., Lopez, L., McElroy, R., Meidt, S. E., Murphy, E .J., Rosolowsky, E., Saito, T., Santoro, F., Schinnerer, E., Schruba, A., Sun, J., Watkins, E. J. and Williams, T. G.
Journal TitleMonthly Notices of the Royal Astronomical Society
Journal Citation508 (4), pp. 5362-5389
Number of Pages28
Year2021
PublisherOxford University Press
Place of PublicationUnited Kingdom
ISSN0035-8711
1365-2966
Digital Object Identifier (DOI)https://doi.org/10.1093/mnras/stab2958
Web Address (URL)https://academic.oup.com/mnras/article/508/4/5362/6402924
Abstract

The feedback from young stars (i.e. pre-supernova) is thought to play a crucial role in molecular cloud destruction. In this paper, we assess the feedback mechanisms acting within a sample of 5810 H II regions identified from the PHANGS-MUSE survey of 19 nearby (<20 Mpc) star-forming, main-sequence spiral galaxies [log(M⋆/M⊙) = 9.4–11]. These optical spectroscopic maps are essential to constrain the physical properties of the H II regions, which we use to investigate their internal pressure terms. We estimate the photoionized gas (Ptherm), direct radiation (Prad), and mechanical wind pressure (Pwind), which we compare to the confining pressure of their host environment (Pde). The H II regions remain unresolved within our ∼50–100 pc resolution observations, so we place upper (Pmax) and lower (Pmin) limits on each of the pressures by using a minimum (i.e. clumpy structure) and maximum (i.e. smooth structure) size, respectively. We find that the Pmax measurements are broadly similar, and for Pmin the Ptherm is mildly dominant. We find that the majority of H II regions are overpressured, Ptot/Pde = (Ptherm + Pwind + Prad)/Pde > 1, and expanding, yet there is a small sample of compact H II regions with Ptot,max/Pde < 1 (∼1 per cent of the sample). These mostly reside in galaxy centres (Rgal < 1 kpc), or, specifically, environments of high gas surface density; log(Σgas/M⊙ pc−2) ∼ 2.5 (measured on kpc-scales). Lastly, we compare to a sample of literature measurements for Ptherm and Prad to investigate how dominant pressure term transitions over around 5 dex in spatial dynamic range and 10 dex in pressure.

KeywordsISM: general; ISM: structure; H II regions; galaxies: ISM; galaxies: star formation
Contains Sensitive ContentDoes not contain sensitive content
ANZSRC Field of Research 2020510102. Astronomical instrumentation
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Byline AffiliationsUniversity of Bonn, Germany
Heidelberg University, Germany
Princeton University, United States
INAF Observatory of Astrophysics and Space Science, Italy
Carnegie Institution for Science, United States
University of Chile, Chile
University of Wyoming, United States
Lomonosov Moscow State University, Russia
European Southern Observatory (ESO), Germany
Australian National University
University of Western Australia
Ohio State University, United States
Liverpool John Moores University, United Kingdom
Max Planck Institute for Astronomy, Germany
University of Gent, Belgium
National Radio Astronomy Observatory, United States
University of Alberta, Canada
Max Planck Institute for Extraterrestrial Physics, Germany
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https://research.usq.edu.au/item/z75v4/comparing-the-pre-sne-feedback-and-environmental-pressures-for-6000-h-ii-regions-across-19-nearby-spiral-galaxies

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The SAMI Galaxy Survey: cubism and covariance, putting round pegs into square holes
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The SAMI Galaxy Survey: Early Data Release
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The SAMI Galaxy Survey: instrument specification and target selection
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Spectroscopic observations of sn 2012fr: A luminous, normal type Ia supernova with early high-velocity features and a late velocity plateau
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The H2O Southern Galactic Plane Survey: NH3 (1,1) and (2,2) catalogues
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The H2O Southern Galactic Plane Survey (HOPS) – I. Techniques and H2O maser data
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A Pilot Survey for the H2O Southern Galactic Plane Survey
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