Molecular emission of CO in BI Cru with high resolution spectroscopy
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F22%3A00562141" target="_blank" >RIV/67985815:_____/22:00562141 - isvavai.cz</a>
Result on the web
<a href="http://www.astronomiaargentina.org.ar/b63/2022BAAA...63..101M.pdf" target="_blank" >http://www.astronomiaargentina.org.ar/b63/2022BAAA...63..101M.pdf</a>
DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
Molecular emission of CO in BI Cru with high resolution spectroscopy
Original language description
In this work we analyze a high-resolution infrared spectrum (R ∼ 45,000) of the symbiotic star BI Cru. This spectrum was obtained using IGRINS spectrograph mounted in Gemini South and ranges from 1.5 to 2.5 μm. From the modeling of the observed CO band emission in the 2.3 μm region, we obtained detailed information of the kinematics and the physical properties of the molecular circumstellar medium.
Czech name
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Czech description
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Classification
Type
J<sub>ost</sub> - Miscellaneous article in a specialist periodical
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GA20-00150S" target="_blank" >GA20-00150S: Structure and evolution of stellar ejecta</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2022
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Boletín de la Asociación Argentina de Astronomía
ISSN
1669-9521
e-ISSN
1669-9521
Volume of the periodical
63
Issue of the periodical within the volume
July
Country of publishing house
AR - ARGENTINA
Number of pages
3
Pages from-to
101-103
UT code for WoS article
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EID of the result in the Scopus database
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