On the huge mass loss of B[e] supergiants in the Magellanic Clouds

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F09%3A00335413" target="_blank" >RIV/67985815:_____/09:00335413 - 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

On the huge mass loss of B[e] supergiants in the Magellanic Clouds

Original language description

B[e] supergiants possess circumstellar disks in which molecules and dust can form. The formation mechanism and the resulting structure of these disks is, however, still controversial. We study the disk dynamics for one B[e] supergiant in the Magellanic Clouds. We find that the disk material must be confined either in an extremely slowly outflowing disk or in a Keplerian rotating ring resulting from a previous ejection event.

Czech name

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Czech description

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Type

D - Article in proceedings

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

Article name in the collection

The Magellanic System: Stars, Gas, and Galaxies

ISBN

978-0-521-88987-2

ISSN

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e-ISSN

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Number of pages

6

Pages from-to

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Publisher name

Cambridge University Press

Place of publication

Cambridge

Event location

Keele

Event date

Jul 28, 2008

Type of event by nationality

WRD - Celosvětová akce

UT code for WoS article

000265876800060