A K-band spectral mini-survey of Galactic B[e] stars

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F14%3A00433398" target="_blank" >RIV/67985815:_____/14:00433398 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1093/mnras/stu1174" target="_blank" >http://dx.doi.org/10.1093/mnras/stu1174</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1093/mnras/stu1174" target="_blank" >10.1093/mnras/stu1174</a>

Result language
angličtina
Original language name
A K-band spectral mini-survey of Galactic B[e] stars
Original language description
We present a mini-survey of Galactic B[e] stars mainly undertaken with the Large Binocular Telescope (LBT). B[e] stars show morphological features with hydrogen emission lines and an infrared excess, attributed to warm circumstellar dust. In general, these features are assumed to arise from dense, non-spherical, disc-forming circumstellar material in which molecules and dust can condensate. We took near-infrared long-slit K-band spectra for a sample of Galactic B[e] stars with the LBT-LUCI 1.
Czech name
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Czech description
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Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2014
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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