Wind and nebula of the M 33 variable GR 290 (WR/LBV)

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F18%3A00494405" target="_blank" >RIV/67985815:_____/18:00494405 - isvavai.cz</a>

Result on the web

<a href="http://dx.doi.org/10.1051/0004-6361/201732540" target="_blank" >http://dx.doi.org/10.1051/0004-6361/201732540</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1051/0004-6361/201732540" target="_blank" >10.1051/0004-6361/201732540</a>

Result language

angličtina

Original language name

Wind and nebula of the M 33 variable GR 290 (WR/LBV)

Original language description

We present a detailed study of this star's wind and mass loss, and a study of the circumstellar environment associated to the star. Long-slit spectra of GR 290 were obtained during its present minimum luminosity phase with the Gran Telescopio Canarias covering the similar to 3600-7500 angstrom wavelength range together with contemporaneous photometry using B, V, R and I filters. The data were compared with non-local thermodynamical equilibrium (non-LTE) model atmosphere synthetic spectra computed with CMFGEN code and with models for ionized interstellar medium regions computed with CLOUDY code.n

Czech name

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Czech description

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Type

J_imp - 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)

Project

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Continuities

Z - Vyzkumny zamer (s odkazem do CEZ)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year

2018

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

Astronomy & Astrophysics

ISSN

1432-0746

e-ISSN

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Volume of the periodical

617

Issue of the periodical within the volume

December

Country of publishing house

FR - FRANCE

Number of pages

12

Pages from-to

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UT code for WoS article

000444811000002

EID of the result in the Scopus database

2-s2.0-85054030172