The IR Compactness of Dusty Galaxies Sets Star Formation and Dust Properties at z 0-2

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A90259%2F23%3A00583714" target="_blank" >RIV/67985815:90259/23:00583714 - isvavai.cz</a>

Result on the web

<a href="https://doi.org/10.3847/1538-4357/ace25c" target="_blank" >https://doi.org/10.3847/1538-4357/ace25c</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.3847/1538-4357/ace25c" target="_blank" >10.3847/1538-4357/ace25c</a>

Result language

angličtina

Original language name

The IR Compactness of Dusty Galaxies Sets Star Formation and Dust Properties at z 0-2

Original language description

The surface densities of gas, dust, and stars provide a window into the physics of star formation that, until the advent of high-resolution far-IR/submillimeter observations, has been historically difficult to assess among dusty galaxies. To study the link between IR surface densities and dust properties, we leverage the Atacama Large Millimetre/Submillimetre Array archive to measure the extent of cold dust emission in 15 z ~ 2 IR-selected galaxies selected on the basis of having available mid-IR spectroscopy from Spitzer.

Czech name

—

Czech description

—

Type

J_imp - Article in a specialist periodical, which is included in the Web of Science database

CEP classification

—

OECD FORD branch

10308 - Astronomy (including astrophysics,space science)

Project

—

Continuities

—

Publication year

2023

Confidentiality

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

Name of the periodical

Astrophysical Journal

ISSN

0004-637X

e-ISSN

1538-4357

Volume of the periodical

955

Issue of the periodical within the volume

2

Country of publishing house

GB - UNITED KINGDOM

Number of pages

17

Pages from-to

136

UT code for WoS article

001122186400001

EID of the result in the Scopus database

2-s2.0-85184797882