Dust around Herbig Ae/Be stars: modelling of observational data

被引：0
作者：
Natalia A. Krivova
Vladimir B. Il’in
Hiroshi Kimura
机构：
[1] Nicholaus Copernicus Astronomical Center,Astronomical Institute
[2] St. Petersburg University,undefined
[3] MPI für Aeronomie,undefined
来源：
Earth, Planets and Space | 1998年 / 50卷
关键词：
Dust; Spectral Energy Distribution; Young Star; Tauri Star; Discrete Dipole Approximation;
D O I：
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学科分类号：
摘要：
Herbig Ae/Be (HAeBe) stars, young stars surrounded by dust shells, are believed to be precursors of β Pic-like stars, and the dust around them is thought to be a possible source material for the formation of planets. A group of the HAeBe stars (UX Ori, WW Vul, etc.) shows large brightness variations. The dust in the vicinity of these stars is responsible not only for their excess emission in the infrared, anomalous extinction in the ultraviolet and visual, and specific spatial distributions of the intensity and polarization, but also for the “blueing” effect in the colour-magnitude diagrams and the intrinsic polarization increase observed in deep minima.
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页码：603 / 606
页数：3
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