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Late O Giants and the Weak Wind Problem

descriptionPublicationkeyboard_double_arrow_right Article , Conference object 01 Jan 2017 France English Publisher:Zenodo
Authors: de Almeida, E. S. G.; Marcolino, W. L. F.; Pereira, C. B.;

doi: 10.5281/zenodo.6480558 , 10.5281/zenodo.6480557

Late O Giants and the Weak Wind Problem

Abstract

We analysed O giants through UV and optical spectroscopy using the code CMFGEN. We conclude that these stars show weak winds and are at the transition region in luminosity for such issue.

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Keywords

[PHYS.ASTR.SR] Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR], stars: winds, stars: fundamental parameters, stars: early-type, stars: mass-loss, outflows

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selected citations
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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).
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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.
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