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International Astronomical Union Colloquium
Article
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International Astronomical Union Colloquium
Article . 1999 . Peer-reviewed
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https://doi.org/10.1007/bfb010...
Part of book or chapter of book . 2008 . Peer-reviewed
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https://dx.doi.org/10.1007/bfb...
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Optical interferometry of non-spherical winds

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Other literature type 01 Jan 1999 English Publisher:Springer Berlin HeidelbergJournal:International Astronomical Union Colloquium, volume 169, pages 87-94 (issn: 0252-9211, Copyright policy )
Authors: Farrokh Vakili; Denis Mourard; Philippe Stee; Daniel Bonneau;

doi: 10.1007/bfb0106359 , 10.1017/s0252921100071815

Optical interferometry of non-spherical winds

Abstract

AbstractOptical Long Baseline Interferometry (OLBI) combined with spectral resolution is capable to sounding the stratification of luminous star winds. In this paper we review some few, yet unique results obtained on P Cyg and Be stars from OLBI observations. We also examine the prospects for studying hot stars winds offered by optical synthesis arrays presently under construction.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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