Fragmentation in the massive G31.41+0.31 protocluster
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F21%3A00553723" target="_blank" >RIV/67985815:_____/21:00553723 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/0004-6361/202040121" target="_blank" >https://doi.org/10.1051/0004-6361/202040121</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/202040121" target="_blank" >10.1051/0004-6361/202040121</a>
Alternative languages
Result language
angličtina
Original language name
Fragmentation in the massive G31.41+0.31 protocluster
Original language description
To establish whether the Main core is indeed monolithic or if its homogeneous appearance is due to a combination of large dust opacity and low angular resolution, we carried out millimeter observations at higher angular resolution and different wavelengths.
Czech name
—
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
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
—
Continuities
—
Others
Publication year
2021
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
648
Issue of the periodical within the volume
April
Country of publishing house
FR - FRANCE
Number of pages
15
Pages from-to
A100
UT code for WoS article
000641867100008
EID of the result in the Scopus database
2-s2.0-85104632277