ALMA reveals a large structured disk and nested rotating outflows in DG Tauri B
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00539618" target="_blank" >RIV/67985815:_____/20:00539618 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.1051/0004-6361/201936950" target="_blank" >https://doi.org/10.1051/0004-6361/201936950</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/0004-6361/201936950" target="_blank" >10.1051/0004-6361/201936950</a>
Alternative languages
Result language
angličtina
Original language name
ALMA reveals a large structured disk and nested rotating outflows in DG Tauri B
Original language description
We present Atacama Large Millimeter Array (ALMA) Band 6 observations at 14-20 au spatial resolution of the disk and CO(2-1) outflow around the Class I protostar DG Tau B in Taurus. The disk is very large, both in dust continuum (R-eff,R- 95% = 174 au) and CO (R-CO = 700 au). It shows Keplerian rotation around a 1.1 +/- 0.2 M-circle dot central star and two dust emission bumps at r = 62 and 135 au. These results confirm that large structured disks can form at an early stage where residual infall is still ongoing.
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
2020
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
1432-0746
e-ISSN
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Volume of the periodical
634
Issue of the periodical within the volume
February
Country of publishing house
FR - FRANCE
Number of pages
11
Pages from-to
L12
UT code for WoS article
000514927300002
EID of the result in the Scopus database
2-s2.0-85089087770