Titlebook: Variable and Non-spherical Stellar Winds in Luminous Hot Stars; Proceedings of the I Bernhard Wolf,Otmar Stahl,Alex W. Fullerton Conference

magnanimity

Anisotropic outflows from LBVs and Ofpe/WN9 stars,tudy of the outflows around evolved massive stars. It has been established (Nota & Clampin 1997) that most LBVs and Ofpe/WN9 stars are surrounded by associated circumstellar nebulae which have been ejected in some previous phase of their evolution. These nebulae are the fossil record of the interact

CHARM

悄悄移動(dòng)

Optical interferometry of non-spherical winds,s paper we review some few, yet unique results obtained on P Cyg and Be stars from OLBI observations. We also examine the prospects for studying hot stars winds offered by optical synthesis arrays presently under construction.

indignant

沉思的魚

d-limonene

Physics of radiatively driven winds by high angular resolution observations (HARO), Hα line profile and continuum energy distribution or polarization data). Nevertheless, little has been done to include High Angular Resolution Observations (HARO) in simulations in spite of the fact that such data can strongly constrain radiative wind models. In the following, we shall review recen

ciliary-body

Wind-compressed disks,s the recently discovered non-radial force components that may inhibit the formation of the disk and present preliminary investigations of the ionization distribution and associated line profiles in the WCD model.

解決

陶瓷

Arrhythmia

Short and medium term variability of emission lines in selected southern Be stars,inct differences between different groups of spectral lines. Based on this empirical phenomenology, a schematic picture of the associated ejection of matter into a near-stellar orbit is sketched and similarities between . Cen and other stars will be outlined.