The Quasi-WR Star HD 45166 Revisited
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00520219" target="_blank" >RIV/67985815:_____/19:00520219 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
The Quasi-WR Star HD 45166 Revisited
Original language description
We studied the wind of the quasi Wolf-Rayet (qWR) star HD 45166. As a first step we modeled the observed UV spectra of this star by means of the state-of-the-art Potsdam Wolf-Rayet (PoWR) atmosphere code. We inferred the wind parameters and compared them with previous findings.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GA16-01116S" target="_blank" >GA16-01116S: Atmospheres and circumstellar environment of magnetic hot stars</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Radiative Signatures from the Cosmos: A Conference in Honor of Ivan Hubený
ISBN
9781583819265
ISSN
1050-3390
e-ISSN
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Number of pages
4
Pages from-to
197-200
Publisher name
Astronomical Society of the Pacific
Place of publication
San Francisco
Event location
Paris
Event date
Oct 23, 2018
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000494866300031