神圣在玷污 发表于 2025-3-28 18:37:13
Monitoring the Winds of Hot Stars with HST/GHRSWe present observations obtained with the Goddard High Resolution Spectrograph (GHRS) of three 0-type stars: ξ per (07 III), λ Cep (06 Iaf) and 10 Lac (09 V). These observations show evidence of instabilities in the winds of all three stars, although not necessarily those expected from current models of structured winds.Cervical-Spine 发表于 2025-3-28 19:53:19
Wolf-Rayet Stars as (Potentially) Fast Rotators with Rotationally-Induced InstabilityIndirect lines of evidence for fast axial rotation of WR stars are described, such as: a) elongated cavities around WRs; b) flattening of WR winds; c) solar-like flares of WRs; d) non-radial pulsations of the WR wind in the presence of a massive companion in a binary system.graphy 发表于 2025-3-29 00:34:22
http://reply.papertrans.cn/47/4680/467914/467914_43.pngnegligence 发表于 2025-3-29 03:53:46
https://doi.org/10.1007/978-94-011-0315-2astrophysics; interstellar matter; simulation; stellar; turbulence; universeCoronary-Spasm 发表于 2025-3-29 10:41:38
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http://reply.papertrans.cn/47/4680/467914/467914_46.pngJAUNT 发表于 2025-3-29 16:05:15
http://reply.papertrans.cn/47/4680/467914/467914_47.pngAffectation 发表于 2025-3-29 21:37:59
http://reply.papertrans.cn/47/4680/467914/467914_48.pngNegotiate 发表于 2025-3-30 03:05:35
http://reply.papertrans.cn/47/4680/467914/467914_49.pngSciatica 发表于 2025-3-30 04:04:05
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