Molecular Gas Properties on Cloud Scales across the Local Star-forming Galaxy Population

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00539712" target="_blank" >RIV/67985815:_____/20:00539712 - isvavai.cz</a>

Result on the web

<a href="https://doi.org/10.3847/2041-8213/abb3be" target="_blank" >https://doi.org/10.3847/2041-8213/abb3be</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.3847/2041-8213/abb3be" target="_blank" >10.3847/2041-8213/abb3be</a>

Result language

angličtina

Original language name

Molecular Gas Properties on Cloud Scales across the Local Star-forming Galaxy Population

Original language description

Using the PHANGS-ALMA CO(2-1) survey, we characterize molecular gas properties on similar to 100 pc scales across 102,778 independent sightlines in 70 nearby galaxies. This yields the best synthetic view of molecular gas properties on cloud scales across the local star-forming galaxy population obtained to date. Consistent with previous studies, we observe a wide range of molecular gas surface densities (3.4 dex), velocity dispersions (1.7 dex), and turbulent pressures (6.5 dex) across the galaxies in our sample.

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

—

Continuities

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Publication year

2020

Confidentiality

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

Name of the periodical

Astrophysical Journal Letters

ISSN

2041-8213

e-ISSN

—

Volume of the periodical

901

Issue of the periodical within the volume

1

Country of publishing house

US - UNITED STATES

Number of pages

12

Pages from-to

L8

UT code for WoS article

000573556500001

EID of the result in the Scopus database

2-s2.0-85092236351