Comparing the Locations of Supernovae to CO (2-1) Emission in Their Host Galaxies
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A90259%2F23%3A00583607" target="_blank" >RIV/67985815:90259/23:00583607 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.3847/1538-4357/acab00" target="_blank" >https://doi.org/10.3847/1538-4357/acab00</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.3847/1538-4357/acab00" target="_blank" >10.3847/1538-4357/acab00</a>
Alternative languages
Result language
angličtina
Original language name
Comparing the Locations of Supernovae to CO (2-1) Emission in Their Host Galaxies
Original language description
We measure the molecular gas environment near recent (<100 yr old) supernovae (SNe) using ~1″ or ≤150 pc resolution CO (2-1) maps from the PHANGS-Atacama Large Millimeter/submillimeter Array (ALMA) survey of nearby star-forming galaxies.
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
Astrophysical Journal
ISSN
0004-637X
e-ISSN
1538-4357
Volume of the periodical
944
Issue of the periodical within the volume
1
Country of publishing house
GB - UNITED KINGDOM
Number of pages
29
Pages from-to
110
UT code for WoS article
000936684700001
EID of the result in the Scopus database
2-s2.0-85148417349