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Variable and Non-spherical Stellar Winds in Luminous Hot Stars: Proceedings of the IAU Colloquium No. 169 Held in Heidelberg, Germany, 1519 June 1998 Softcover reprint of the original 1st ed. 1999 [Pehme köide]

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  • Formaat: Paperback / softback, 428 pages, kõrgus x laius: 235x155 mm, kaal: 688 g, 171 Illustrations, black and white; XX, 428 p. 171 illus., 1 Paperback / softback
  • Sari: Lecture Notes in Physics 523
  • Ilmumisaeg: 23-Aug-2014
  • Kirjastus: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
  • ISBN-10: 3662142104
  • ISBN-13: 9783662142103
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  • Formaat: Paperback / softback, 428 pages, kõrgus x laius: 235x155 mm, kaal: 688 g, 171 Illustrations, black and white; XX, 428 p. 171 illus., 1 Paperback / softback
  • Sari: Lecture Notes in Physics 523
  • Ilmumisaeg: 23-Aug-2014
  • Kirjastus: Springer-Verlag Berlin and Heidelberg GmbH & Co. K
  • ISBN-10: 3662142104
  • ISBN-13: 9783662142103
There is abundant evidence that essentially all luminous hot-star winds contain time-dependent and anisotropic structures. IAU Colloquium 169 was convened to review the observations of variability and asphericity, to discuss the physical processes that might cause such behavior and to look for evolutionary consequences. The topics included OBA stars, Be stars, Wolf-Rayet stars, Be stars, and luminous blue variables (LBVs). The role played by rotation in shaping the stellar wind was a recurrent theme. Photospheric pulsations and/or magnetic fields are particularly appealing mechanisms for triggering the formation of recurrent wind structures.

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Rotationally modulated winds of O stars.- Rotationally modulated winds
of BA-type supergiants.- Using spectropolarimetry to determine envelope
geometry and test variability models for hot star circumstellar envelopes.-
Disks of classical be stars.- Evidence for azimuthal asymmetry in be star
winds.- Short and medium term variability of emission lines in selected
southern Be stars.- Disk winds of B[ e] supergiants.- Polarimetric evidence of
non-spherical winds.- Wolf-rayet wind models: Photometric and polarimetric
variability.- Anisotropic outflows from LBVs and Ofpe/WN9 stars.-
Non-isotropic outflows in the infrared: ISO imaging of LBVs.- Radio evidence
for non-isotropic outflows from hot stars.- Optical interferometry of
non-spherical winds.- Direct observational evidence for magnetic fields in
hot stars.- HST WFPCII observations of the inner HR car nebula.- Observing
hot stars in all four stokes parameters.- Inverse spectropolarimetric
modelling of hot star wind structure and variability.- Physics of radiatively
driven winds by high angular resolution observations (HARO).- Wind-compressed
disks.- Non-spherical radiation-driven wind models.- Radiation-driven disk
winds.- Radiative fluxes and forces in non-spherical winds.- Line-driven
ablation by external irradiation.- Extremely luminous atmospheres.- Disks
formed by rotation induced bi-stability.- The effects of magnetic fields on
the winds from luminous hot stars.- Modeling oblique rotators: Magnetospheres
and winds.- X-ray emission from magnetically confined winds.- O-star wind
variability in the ultraviolet and optical range.- X-ray evidence for wind
instabilities.- X-ray variability of the O star ? Puppis.- On the variable
winds of BA supergiants.- UV wind variability in B supergiants and its
implications for windstructures.- Variability and evidence of non-spherical
stellar winds in A-type supergiants.- Variable winds in early-B hypergiants.-
Wind variations of wolf-rayet stars.- Spectral analyses of wolf-rayet stars:
The impact of clumping.- The long-term variability of luminous blue
variables.- Blitz model for the eruptions of eta carinae.- Short-term
variations of LBVs.- Imaging polarimetry of eta carinae with the hubble
space telescope.- Non-spherical outflows in massive binary systems:
Circumbinary disks?.- Long-term behaviour of the variable wind of P Cygni.-
High-resolution spectroscopy of stellar winds in recently recognized LBV
candidates.- Evidence for wind anisotropies from dust formation by wolf-rayet
stars.- ISO-SWS spectroscopy of B[ e] stars.- The line-driven instability.-
Co-rotating interaction regions in 2D hot-star wind models with line-driven
instability.- Pulsations in O stars.- Non-radial pulsations of BA supergiants
and Be stars.- Theory of pulsational instabilities of hot stars.-
Non-radially pulsating hot stars: Non-radial pulsations and Be phenomenon.-
Pulsation hydrodynamics of luminous blue variables and pulsation-driven
winds.- Linear strange modes in massive stars.- Instabilities in LBVs and WR
stars.- The evolution of non-spherical and non-stationary winds of massive
stars.- Rotation and anisotropic losses of mass and angular momentum.-
Rotation and wolf-rayet star formation.- Dusty LBV nebulae: Tracing the mass
loss history of the most massive stars.- Wolf-rayet and LBV nebulae as the
result of variable and non-spherical stellar winds.- Ring nebulae abundances:
Probes of the evolutionary history of luminous blue variable stars.- The wind
momentum Luminosity relationship of blue supergiants.- Conference summary:
The demise of spherical andstationary winds.