About: Macroclumping as solution of the discrepancy between Hα and P v mass loss diagnostics for O-type stars     Goto   Sponge   NotDistinct   Permalink

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  • In a previous paper, we presented 3D Monte-Carlo calculations for the formation of scattering lines in a clumped stellar wind. In the present paper we select five O-type supergiants (from O4 to O7) and test whether the reported discrepancies can be resolved this way. Our results show that with the mass-loss rates that fit Hα (and other Balmer and He ii lines), the UV resonance lines (especially the unsaturated doublet of P v) can also be reproduced with no problem when macroclumping is taken into account. There is no need to artificially reduce the mass-loss rates or to assume a subsolar phosphorus abundance or an extremely high clumping factor, unlike what was claimed by other authors. These consistent mass-loss rates are lower by a factor of 1.3 to 2.6, compared to the mass-loss rate recipe from Vink et al.
  • In a previous paper, we presented 3D Monte-Carlo calculations for the formation of scattering lines in a clumped stellar wind. In the present paper we select five O-type supergiants (from O4 to O7) and test whether the reported discrepancies can be resolved this way. Our results show that with the mass-loss rates that fit Hα (and other Balmer and He ii lines), the UV resonance lines (especially the unsaturated doublet of P v) can also be reproduced with no problem when macroclumping is taken into account. There is no need to artificially reduce the mass-loss rates or to assume a subsolar phosphorus abundance or an extremely high clumping factor, unlike what was claimed by other authors. These consistent mass-loss rates are lower by a factor of 1.3 to 2.6, compared to the mass-loss rate recipe from Vink et al. (en)
Title
  • Macroclumping as solution of the discrepancy between Hα and P v mass loss diagnostics for O-type stars
  • Macroclumping as solution of the discrepancy between Hα and P v mass loss diagnostics for O-type stars (en)
skos:prefLabel
  • Macroclumping as solution of the discrepancy between Hα and P v mass loss diagnostics for O-type stars
  • Macroclumping as solution of the discrepancy between Hα and P v mass loss diagnostics for O-type stars (en)
skos:notation
  • RIV/67985815:_____/13:00424407!RIV14-MSM-67985815
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  • I, P(7AMB12AR021), P(GAP209/11/1198)
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  • November
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  • 85662
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  • RIV/67985815:_____/13:00424407
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  • stars; winds; outflows (en)
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  • FR - Francouzská republika
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  • [EA12FB1A7BF6]
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  • Astronomy & Astrophysics
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  • 559
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  • Kubát, Jiří
  • Šurlan, Brankica
  • Hamann, W.-R.
  • Oskinova, L. M.
  • Torres, A. F.
  • Aret, A.
http://linked.open...ain/vavai/riv/wos
  • 000327847200130
issn
  • 0004-6361
number of pages
http://bibframe.org/vocab/doi
  • 10.1051/0004-6361/201322390
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