On the Role of the WNH Phase in the Evolution of Very Massive Stars: Enabling the LBV Instability with Feedback
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The evolution of massive stars and their spectra. I. A non-rotating 60 M_{sun}_ star from the zero-age main sequence to the pre-supernova stageOn the nature of the galactic early-B hypergiantsTwo extremely luminous WN stars in the Galactic center with circumstellar emission from dust and gasThe Galactic WC starsSpectral classification of O2-3.5 If*/WN5-7 starsLuminous blue variable eruptions and related transients: diversity of progenitors and outburst propertiesA Galactic O2 If*/WN6 star possibly ejected from its birthplace in NGC 3603The Quintuplet cluster
P2860
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P2860
On the Role of the WNH Phase in the Evolution of Very Massive Stars: Enabling the LBV Instability with Feedback
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Juni 2008 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
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наукова стаття, опублікована в червні 2008
@uk
name
On the Role of the WNH Phase i ...... LBV Instability with Feedback
@en
On the Role of the WNH Phase i ...... LBV Instability with Feedback
@nl
type
label
On the Role of the WNH Phase i ...... LBV Instability with Feedback
@en
On the Role of the WNH Phase i ...... LBV Instability with Feedback
@nl
prefLabel
On the Role of the WNH Phase i ...... LBV Instability with Feedback
@en
On the Role of the WNH Phase i ...... LBV Instability with Feedback
@nl
P356
P1476
On the Role of the WNH Phase i ...... LBV Instability with Feedback
@en
P2093
Nathan Smith
Peter S. Conti
P304
P356
10.1086/586885
P407
P577
2008-06-01T00:00:00Z
P5875
P818
P819
2008ApJ...679.1467S