File:Protoplanetary disk.svg

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Русский: Теоретическое изображение протопланетного диска на длинах волн 3 мм (левая карта) и 160 микрон (правая карта). Ось диска наклонена к наблюдателю под углом 75 градусов. Изображения получены по результатам моделирования динамики самогравитирующего газопылевого диска и расчета переноса излучения. Справа от центра присутствует плотный фрагмент --- зародыш планеты. На длине волны 3 мм, в которой диск прозрачен, этот фрагмент наблюдается в виде пятна повышенной яркости (левая карта). На длине 160 мкм, в котором диск является оптически толстым, фрагмент проявляется в виде темной области (правая карта).
English: The theoretical images of a protoplanetary disk at 3 mm (left map) and 160 micron (right map). The angle between the axis of the disk and an observer is 75 degree. The images are produced as a result of protoplanetary disk simulations with a hydrodynamical and radiative transfer models. To the right from the center one can see a dense fragment which is going to form a protoplanet. The disk is transparent in 3 mm so this fragment appears as a bright spot in the left map. The optical depth of the disk is significant in 160 micron so the fragment manifests itself as a dark region on the right map.
Date
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Author Yaroslav Pavlyuchenkov

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28 December 2015

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Date/TimeThumbnailDimensionsUserComment
current16:52, 17 March 2016Thumbnail for version as of 16:52, 17 March 2016990 × 765 (7.56 MB)Maxinvestigatorfail upload
16:48, 17 March 2016Thumbnail for version as of 16:48, 17 March 2016864 × 511 (9.91 MB)Maxinvestigatoralignment, cropped
12:09, 28 December 2015Thumbnail for version as of 12:09, 28 December 2015990 × 765 (7.56 MB)PavyarUser created page with UploadWizard

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