The gas morphology of nearby star-forming galaxies
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A90259%2F23%3A00583709" target="_blank" >RIV/67985815:90259/23:00583709 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/0004-6361/202346318" target="_blank" >https://doi.org/10.1051/0004-6361/202346318</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202346318" target="_blank" >10.1051/0004-6361/202346318</a>
Alternative languages
Result language
angličtina
Original language name
The gas morphology of nearby star-forming galaxies
Original language description
A galaxy's morphology stems from the secular and environmental processes taking place over the course of its evolutionary history. Thus, it has consistently served as an important tool for gaining insights into galaxy evolution. In this work, we visually classified morphologies on cloud-scales based on the molecular gas distribution of a large sample of 79 nearby main sequence galaxies, using 1″ resolution CO(2-1) ALMA observations taken as part of the PHANGS survey.
Czech name
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Czech description
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Classification
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)
Result continuities
Project
—
Continuities
—
Others
Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomy & Astrophysics
ISSN
0004-6361
e-ISSN
1432-0746
Volume of the periodical
676
Issue of the periodical within the volume
August
Country of publishing house
FR - FRANCE
Number of pages
26
Pages from-to
A113
UT code for WoS article
001050856400013
EID of the result in the Scopus database
2-s2.0-85169037565