WISDOM Project - X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00569261" target="_blank" >RIV/67985815:_____/22:00569261 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1093/mnras/stac600" target="_blank" >https://doi.org/10.1093/mnras/stac600</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnras/stac600" target="_blank" >10.1093/mnras/stac600</a>

Result language
angličtina
Original language name
WISDOM Project - X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure
Original language description
We use high-resolution maps of the molecular interstellar medium (ISM) in the centres of 86 nearby galaxies from the millimetre-Wave Interferometric Survey of Dark Object Masses (WISDOM) and Physics at High Angular Resolution in Nearby GalaxieS (PHANGS) surveys to investigate the physical mechanisms setting the morphology of the ISM at molecular cloud scales. We show that early-type galaxies tend to have smooth, regular molecular gas morphologies, while the ISM in spiral galaxy bulges is much more asymmetric and clumpy when observed at the same spatial scales.
Czech name
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Czech description
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Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)

Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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