PHANGS-JWST First Results: Dust-embedded Star Clusters in NGC 7496 Selected via 3.3 μm PAH Emission

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A90259%2F23%3A00583931" target="_blank" >RIV/67985815:90259/23:00583931 - isvavai.cz</a>

Result on the web

<a href="https://doi.org/10.3847/2041-8213/aca653" target="_blank" >https://doi.org/10.3847/2041-8213/aca653</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.3847/2041-8213/aca653" target="_blank" >10.3847/2041-8213/aca653</a>

Result language

angličtina

Original language name

PHANGS-JWST First Results: Dust-embedded Star Clusters in NGC 7496 Selected via 3.3 μm PAH Emission

Original language description

Here we leverage the extraordinary new high-resolution infrared imaging from JWST to begin the study of dust-embedded star clusters in nearby galaxies throughout the Local Volume. We present a technique for identifying dust-embedded clusters in NGC 7496 (18.7 Mpc), the first galaxy to be observed by the PHANGS-JWST Cycle 1 Treasury Survey. We select sources that have strong 3.3 μm PAH emission based on a F300M - F335M color excess and identify 67 candidate embedded clusters.

Czech name

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Czech description

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Type

J_imp - 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)

Project

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Continuities

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Publication year

2023

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Astrophysical Journal Letters

ISSN

2041-8205

e-ISSN

2041-8213

Volume of the periodical

944

Issue of the periodical within the volume

2

Country of publishing house

US - UNITED STATES

Number of pages

10

Pages from-to

L26

UT code for WoS article

000941973200001

EID of the result in the Scopus database

2-s2.0-85148760265