File:Proplyd NGC 6193.png

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Proplyd_NGC_6193.png(438 × 456 pixels, file size: 149 KB, MIME type: image/png)

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English: Dusty proplyds in the star cluster NGC 6193, which appears as a star leaving a red tail behind. The external evaporation of dust from the disk of this object is caused by nearby OB-stars. The dust is then swept away by the nearby OB-stars HD 150136 and CD-48 11071 , forming a tail in the wake of the young stars.

Image Credit: NASA Spitzer Space Telescope

Filters: 4.5, 8.0 and 24 Micron
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Source Own work
Author Meli thev

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Date/TimeThumbnailDimensionsUserComment
current17:43, 15 May 2023Thumbnail for version as of 17:43, 15 May 2023438 × 456 (149 KB)Meli thev (talk | contribs)Uploaded own work with UploadWizard

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