Spectroscopic study of the B[e] supergiant LHA 120-S 35

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F12%3A00424010" target="_blank" >RIV/67985815:_____/12:00424010 - isvavai.cz</a>

Result on the web

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DOI - Digital Object Identifier

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Result language

angličtina

Original language name

Spectroscopic study of the B[e] supergiant LHA 120-S 35

Original language description

LHA 120-S 35 is a poorly studied supergiant of the Large Magellanic Cloud which displays the B[e] phenomenon. In this work, we present a spectroscopic description of this star based on high-resolution optical spectra (3600 to 9200 ?), taken with the Du Pont Telescope at Las Campanas Observatory (LCO), Chile. In addition, we obtained medium resolution K-band near infrared spectra for this object with SINFONI on the VLT UT4 telescope at the European Southern Observatory (ESO). The near infrared spectra show strong CO band emission. This is the first detection of molecular emission in this peculiar star.

Czech name

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Czech description

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Type

J_x - 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

2012

Confidentiality

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

Name of the periodical

Boletín de la Asociación Argentina de Astronomía

ISSN

1669-9521

e-ISSN

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Volume of the periodical

55

Issue of the periodical within the volume

1

Country of publishing house

AR - ARGENTINA

Number of pages

4

Pages from-to

155-158

UT code for WoS article

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EID of the result in the Scopus database

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