Oscar Agertz
Associate Professor / Senior university lecturer / Wallenberg Academy Fellow
Physical properties and scaling relations of molecular clouds : The effect of stellar feedback
Author
Summary, in English
Using hydrodynamical simulations of entire galactic discs similar to the Milky Way (MW), reaching 4.6 pc resolution, we study the origins of observed physical properties of giant molecular clouds (GMCs). We find that efficient stellar feedback is a necessary ingredient in order to develop a realistic interstellar medium, leading to molecular cloud masses, sizes, velocity dispersions, and virial parameters in excellent agreement withMWobservations. GMCscaling relations observed in the MW, such as the mass-size (M-R), velocity dispersion-size (σ-R), and the σ-RΣ relations, are reproduced in a feedback-driven ISM when observed in projection, with M∝R2.3 and σ∝R0.56.When analysed in 3D, GMC scaling relations steepen significantly, indicating potential limitations of our understanding of molecular cloud 3D structure from observations. Furthermore, we demonstrate how a GMC population's underlying distribution of virial parameters can strongly influence the scatter in derived scaling relations. Finally, we show that GMCs with nearly identical global properties exist in different evolutionary stages, where a majority of clouds being either gravitationally bound or expanding, but with a significant fraction being compressed by external ISM pressure, at all times.
Department/s
- Lund Observatory - Has been reorganised
Publishing year
2018-09-21
Language
English
Pages
3167-3180
Publication/Series
Monthly Notices of the Royal Astronomical Society
Volume
479
Issue
3
Document type
Journal article
Publisher
Oxford University Press
Topic
- Astronomy, Astrophysics and Cosmology
Keywords
- Galaxies:evolution
- Galaxies:formation
- Galaxies:ism
- Galaxies:structure
Status
Published
ISBN/ISSN/Other
- ISSN: 0035-8711