An interferometric view of hot star disks

An interferometric view of hot star disks

Optical long baseline interferometry was recently established as a technique capable of resolving stars and their circumstellar environments at the milliarcsecond (mas) resolution level. This high-resolution opens an entire new window to the study of astrophysical systems, providing information...

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Bibliographic Details
Main Author: Daniel Moser Faes
Other Authors: Alex Cavalieri Carciofi
Language:English
Published: Universidade de São Paulo 2015
Subjects:
estrelas: campo magnético
estrelas: individual (Achernar)
estrelas: linha de emissão - Be
estrelas: parâmetros fundamentais
material circunstelar
técnicas: interferométrica
circumstellar matter
individual (Achernar)
stars: emission-line - Be
stars: fundamental parameters
stars: magnetic field
techniques: interferometric
Online Access:http://www.teses.usp.br/teses/disponiveis/14/14131/tde-16122015-201029/

Internet

http://www.teses.usp.br/teses/disponiveis/14/14131/tde-16122015-201029/

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