Resolved stellar population properties of PHANGS-MUSE galaxies
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A90259%2F23%3A00583796" target="_blank" >RIV/67985815:90259/23:00583796 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/0004-6361/202245673" target="_blank" >https://doi.org/10.1051/0004-6361/202245673</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202245673" target="_blank" >10.1051/0004-6361/202245673</a>
Alternative languages
Result language
angličtina
Original language name
Resolved stellar population properties of PHANGS-MUSE galaxies
Original language description
We present a detailed analysis of the spatially resolved star formation histories (SFHs) of 19 PHANGS-MUSE galaxies, at a spatial resolution of ∼100 pc. We show that our sample of local galaxies exhibits predominantly negative radial gradients of stellar age and metallicity, consistent with previous findings, and a radial structure that is primarily consistent with local star formation, and indicative of inside-out formation.
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
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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
673
Issue of the periodical within the volume
May
Country of publishing house
FR - FRANCE
Number of pages
49
Pages from-to
A147
UT code for WoS article
000996517500003
EID of the result in the Scopus database
2-s2.0-85161088704