Star formation scaling relations at similar to 100 pc from PHANGS: Impact of completeness and spatial scale
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F21%3A00553813" target="_blank" >RIV/67985815:_____/21:00553813 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/0004-6361/202140733" target="_blank" >https://doi.org/10.1051/0004-6361/202140733</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202140733" target="_blank" >10.1051/0004-6361/202140733</a>
Alternative languages
Result language
angličtina
Original language name
Star formation scaling relations at similar to 100 pc from PHANGS: Impact of completeness and spatial scale
Original language description
he complexity of star formation at the physical scale of molecular clouds is not yet fully understood. We investigate the mechanisms regulating the formation of stars in different environments within nearby star-forming galaxies from the Physics at High Angular resolution in Nearby GalaxieS (PHANGS) sample.
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
2021
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
650
Issue of the periodical within the volume
June
Country of publishing house
FR - FRANCE
Number of pages
26
Pages from-to
A134
UT code for WoS article
000668709400001
EID of the result in the Scopus database
2-s2.0-85108543509