Diagnosing 0.1-10 au Scale Morphology of the FU Ori Disk Using ALMA and VLTI/GRAVITY
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00539881" target="_blank" >RIV/67985815:_____/19:00539881 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.3847/1538-4357/ab391c" target="_blank" >https://doi.org/10.3847/1538-4357/ab391c</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.3847/1538-4357/ab391c" target="_blank" >10.3847/1538-4357/ab391c</a>
Alternative languages
Result language
angličtina
Original language name
Diagnosing 0.1-10 au Scale Morphology of the FU Ori Disk Using ALMA and VLTI/GRAVITY
Original language description
We report new Atacama Large Millimeter/submillimeter Array Band 3 (86-100 GHz, similar to 80 mas angular resolution) and Band 4 (146-160 GHz, similar to 50 mas angular resolution) observations of the dust continuum emission toward the archetypal and ongoing accretion burst young stellar object FU Ori, which simultaneously covered its companion, FU Ori S. In addition, we present near-infrared (2-2.45 mu m) observations of FU Ori taken with the General Relativity Analysis via VLT InTerferometrY (GRAVITY, similar to 1 mas angular resolution) instrument on the Very Large Telescope Interferometer (VLTI).
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
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Continuities
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Others
Publication year
2019
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
1538-4357
e-ISSN
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Volume of the periodical
884
Issue of the periodical within the volume
1
Country of publishing house
US - UNITED STATES
Number of pages
13
Pages from-to
97
UT code for WoS article
000501733600022
EID of the result in the Scopus database
2-s2.0-85073827683