magnanimity
发表于 2025-3-30 08:20:58
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
发表于 2025-3-30 15:53:38
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悄悄移动
发表于 2025-3-30 17:27:31
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
发表于 2025-3-30 21:08:32
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沉思的鱼
发表于 2025-3-31 01:01:58
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d-limonene
发表于 2025-3-31 07:31:16
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
发表于 2025-3-31 10:41:41
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.
解决
发表于 2025-3-31 13:42:06
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陶瓷
发表于 2025-3-31 19:56:14
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Arrhythmia
发表于 2025-3-31 23:42:31
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.