The pre- versus post-main sequence evolutionary phase of B[e] stars. Constraints from 13CO band emission

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F09%3A00335404" target="_blank" >RIV/67985815:_____/09:00335404 - 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

The pre- versus post-main sequence evolutionary phase of B[e] stars. Constraints from 13CO band emission

Original language description

The many similarities between pre-main sequence (Herbig) stars and evolved supergiant stars hamper proper stellar classifications of galactic B[e] objects significantly. We propose a new classification characetristic to distinguish these two groups unambiguously, based on the appearance of 13CO band emission. We show that the detection of 13CO band head emission in medium-resolution K-band spectra of B[e] stars is an immediate proof for an evolved (supergiant) nature of the 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

<a href="/en/project/KJB300030701" target="_blank" >KJB300030701: B[e] supergiants: where is their place within the evolution of massive stars?</a><br>

Continuities

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)

Publication year

2009

Confidentiality

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

Name of the periodical

Astronomy and Astrophysics

ISSN

0004-6361

e-ISSN

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Volume of the periodical

494

Issue of the periodical within the volume

1

Country of publishing house

FR - FRANCE

Number of pages

10

Pages from-to

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UT code for WoS article

000263040200021

EID of the result in the Scopus database

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