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Calculation of the masses of the binary star HD 93205 by application of the theory of apsidal motionBright OB stars in the Galaxy. IV. Stellar and wind parameters of early to late B supergiantsThe R136 star cluster dissected withHubble Space Telescope/STIS. I. Far-ultraviolet spectroscopic census and the origin of He ii λ1640 in young star clustersThe emergence of super-canonical stars in R136-type starburst clustersAxi-symmetric models of B[e] supergiants. I. The effective temperature and mass-loss dependence of the hydrogen and helium ionization structureThe VLT-FLAMES Tarantula SurveyThe VLT-FLAMES Tarantula SurveyOn the possibility that the most massive stars result from binary mergersThe VLT-FLAMES Tarantula SurveyThe VLT-FLAMES Tarantula SurveyThe VLT-FLAMES Tarantula SurveyThe VLT-FLAMES Tarantula SurveyThe VLT-FLAMES Tarantula SurveyThe VLT-FLAMES Tarantula SurveyBinary-corrected velocity dispersions from single- and multi-epoch radial velocities: massive stars in R136 as a test caseNo breakdown of the radiatively driven wind theory in low-metallicity environments★†
P2860
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P2860
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Dezember 1998 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в грудні 1998
@uk
name
An Empirical Isochrone of Very Massive Stars in R136a
@en
An Empirical Isochrone of Very Massive Stars in R136a
@nl
type
label
An Empirical Isochrone of Very Massive Stars in R136a
@en
An Empirical Isochrone of Very Massive Stars in R136a
@nl
prefLabel
An Empirical Isochrone of Very Massive Stars in R136a
@en
An Empirical Isochrone of Very Massive Stars in R136a
@nl
P2093
P356
P1476
An Empirical Isochrone of Very Massive Stars in R136a
@en
P2093
Alex de Koter
Ivan Hubeny
Sara R. Heap
P304
P356
10.1086/306503
P407
P577
1998-12-20T00:00:00Z
P5875
P819
1998ApJ...509..879D