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 | |
| Source | Own work |
| Author | Yaroslav Pavlyuchenkov |
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I, the copyright holder of this work, hereby publish it under the following license:
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This image was uploaded as part of European Science Photo Competition 2015. |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 16:52, 17 March 2016 | | 990 × 765 (7.56 MB) | Maxinvestigator (talk | contribs) | fail upload |
| 16:48, 17 March 2016 |  | 864 × 511 (9.91 MB) | Maxinvestigator (talk | contribs) | alignment, cropped | |
| 12:09, 28 December 2015 |  | 990 × 765 (7.56 MB) | Pavyar (talk | contribs) | User created page with UploadWizard |
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